Coverage for pygeodesy/ellipsoids.py: 96%

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1 

2# -*- coding: utf-8 -*- 

3 

4u'''Ellipsoidal and spherical earth models. 

5 

6Classes L{a_f2Tuple}, L{Ellipsoid} and L{Ellipsoid2}, an L{Ellipsoids} registry and 

72 dozen functions to convert I{equatorial} radius, I{polar} radius, I{eccentricities}, 

8I{flattenings} and I{inverse flattening}. 

9 

10See module L{datums} for L{Datum} and L{Transform} information and other details. 

11 

12Following is the list of predefined L{Ellipsoid}s, all instantiated lazily. 

13 

14@var Ellipsoids.Airy1830: Ellipsoid(name='Airy1830', a=6377563.396, b=6356256.90923729, f_=299.3249646, f=0.00334085, f2=0.00335205, n=0.00167322, e=0.08167337, e2=0.00667054, e21=0.99332946, e22=0.00671533, e32=0.00334643, A=6366914.60892522, L=10001126.0807165, R1=6370461.23374576, R2=6370459.65470808, R3=6370453.30994572, Rbiaxial=6366919.065224, Rtriaxial=6372243.45317691) 

15@var Ellipsoids.AiryModified: Ellipsoid(name='AiryModified', a=6377340.189, b=6356034.44793853, f_=299.3249646, f=0.00334085, f2=0.00335205, n=0.00167322, e=0.08167337, e2=0.00667054, e21=0.99332946, e22=0.00671533, e32=0.00334643, A=6366691.77461988, L=10000776.05340819, R1=6370238.27531284, R2=6370236.69633043, R3=6370230.35179013, Rbiaxial=6366696.2307627, Rtriaxial=6372020.43236847) 

16@var Ellipsoids.ATS1977: Ellipsoid(name='ATS1977', a=6378135, b=6356750.30492159, f_=298.257, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181922, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367447.14116695, L=10001962.58040571, R1=6371006.7683072, R2=6371005.17780873, R3=6370998.78689182, Rbiaxial=6367451.62986519, Rtriaxial=6372795.55363648) 

17@var Ellipsoids.Australia1966: Ellipsoid(name='Australia1966', a=6378160, b=6356774.71919531, f_=298.25, f=0.00335289, f2=0.00336417, n=0.00167926, e=0.08182018, e2=0.00669454, e21=0.99330546, e22=0.00673966, e32=0.00335851, A=6367471.84853228, L=10002001.39064442, R1=6371031.5730651, R2=6371029.9824858, R3=6371023.59124344, Rbiaxial=6367476.337459, Rtriaxial=6372820.40754721) 

18@var Ellipsoids.Bessel1841: Ellipsoid(name='Bessel1841', a=6377397.155, b=6356078.962818, f_=299.1528128, f=0.00334277, f2=0.00335398, n=0.00167418, e=0.08169683, e2=0.00667437, e21=0.99332563, e22=0.00671922, e32=0.00334836, A=6366742.52023395, L=10000855.76443237, R1=6370291.09093933, R2=6370289.51012659, R3=6370283.15821523, Rbiaxial=6366746.98155108, Rtriaxial=6372074.29334012) 

19@var Ellipsoids.BesselModified: Ellipsoid(name='BesselModified', a=6377492.018, b=6356173.5087127, f_=299.1528128, f=0.00334277, f2=0.00335398, n=0.00167418, e=0.08169683, e2=0.00667437, e21=0.99332563, e22=0.00671922, e32=0.00334836, A=6366837.22474766, L=10001004.52593463, R1=6370385.84823756, R2=6370384.26740131, R3=6370377.91539546, Rbiaxial=6366841.68613115, Rtriaxial=6372169.07716325) 

20@var Ellipsoids.CGCS2000: Ellipsoid(name='CGCS2000', a=6378137, b=6356752.31414036, f_=298.2572221, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367449.14577105, L=10001965.72923046, R1=6371008.77138012, R2=6371007.18088352, R3=6371000.78997414, Rbiaxial=6367453.63446401, Rtriaxial=6372797.55593326) 

21@var Ellipsoids.Clarke1866: Ellipsoid(name='Clarke1866', a=6378206.4, b=6356583.8, f_=294.97869821, f=0.00339008, f2=0.00340161, n=0.00169792, e=0.08227185, e2=0.00676866, e21=0.99323134, e22=0.00681478, e32=0.00339582, A=6367399.68916978, L=10001888.04298286, R1=6370998.86666667, R2=6370997.240633, R3=6370990.70659881, Rbiaxial=6367404.2783313, Rtriaxial=6372807.62791066) 

22@var Ellipsoids.Clarke1880: Ellipsoid(name='Clarke1880', a=6378249.145, b=6356514.86954978, f_=293.465, f=0.00340756, f2=0.00341921, n=0.00170669, e=0.0824834, e2=0.00680351, e21=0.99319649, e22=0.00685012, e32=0.00341337, A=6367386.64398051, L=10001867.55164747, R1=6371004.38651659, R2=6371002.74366963, R3=6370996.1419165, Rbiaxial=6367391.2806777, Rtriaxial=6372822.52526083) 

23@var Ellipsoids.Clarke1880IGN: Ellipsoid(name='Clarke1880IGN', a=6378249.2, b=6356515, f_=293.46602129, f=0.00340755, f2=0.0034192, n=0.00170668, e=0.08248326, e2=0.00680349, e21=0.99319651, e22=0.00685009, e32=0.00341336, A=6367386.73667336, L=10001867.69724907, R1=6371004.46666667, R2=6371002.82383112, R3=6370996.22212395, Rbiaxial=6367391.37333829, Rtriaxial=6372822.59907505) 

24@var Ellipsoids.Clarke1880Mod: Ellipsoid(name='Clarke1880Mod', a=6378249.145, b=6356514.96639549, f_=293.46630766, f=0.00340755, f2=0.0034192, n=0.00170668, e=0.08248322, e2=0.00680348, e21=0.99319652, e22=0.00685009, e32=0.00341335, A=6367386.69236201, L=10001867.62764496, R1=6371004.4187985, R2=6371002.77596616, R3=6370996.17427195, Rbiaxial=6367391.32901784, Rtriaxial=6372822.5494103) 

25@var Ellipsoids.CPM1799: Ellipsoid(name='CPM1799', a=6375738.7, b=6356671.92557493, f_=334.39, f=0.00299052, f2=0.00299949, n=0.0014975, e=0.07727934, e2=0.0059721, e21=0.9940279, e22=0.00600798, e32=0.00299499, A=6366208.88184784, L=10000017.52721564, R1=6369383.10852498, R2=6369381.8434158, R3=6369376.76247022, Rbiaxial=6366212.45090321, Rtriaxial=6370977.3559758) 

26@var Ellipsoids.Delambre1810: Ellipsoid(name='Delambre1810', a=6376428, b=6355957.92616372, f_=311.5, f=0.00321027, f2=0.00322061, n=0.00160772, e=0.08006397, e2=0.00641024, e21=0.99358976, e22=0.0064516, e32=0.00321543, A=6366197.07684334, L=9999998.98395793, R1=6369604.64205457, R2=6369603.18419749, R3=6369597.32739068, Rbiaxial=6366201.19059818, Rtriaxial=6371316.64722284) 

27@var Ellipsoids.Engelis1985: Ellipsoid(name='Engelis1985', a=6378136.05, b=6356751.32272154, f_=298.2566, f=0.00335282, f2=0.0033641, n=0.00167922, e=0.08181928, e2=0.00669439, e21=0.99330561, e22=0.00673951, e32=0.00335844, A=6367448.17507971, L=10001964.20447208, R1=6371007.80757385, R2=6371006.21707085, R3=6370999.82613573, Rbiaxial=6367452.66379074, Rtriaxial=6372796.59560563) 

28@var Ellipsoids.Everest1969: Ellipsoid(name='Everest1969', a=6377295.664, b=6356094.667915, f_=300.8017, f=0.00332445, f2=0.00333554, n=0.00166499, e=0.08147298, e2=0.00663785, e21=0.99336215, e22=0.0066822, e32=0.00332998, A=6366699.57839501, L=10000788.3115495, R1=6370228.665305, R2=6370227.10178537, R3=6370220.81951618, Rbiaxial=6366703.99082487, Rtriaxial=6372002.02812501) 

29@var Ellipsoids.Everest1975: Ellipsoid(name='Everest1975', a=6377299.151, b=6356098.14512013, f_=300.8017255, f=0.00332445, f2=0.00333554, n=0.00166499, e=0.08147298, e2=0.00663785, e21=0.99336215, e22=0.0066822, e32=0.00332997, A=6366703.06049924, L=10000793.78122603, R1=6370232.14904004, R2=6370230.58551983, R3=6370224.30324826, Rbiaxial=6366707.47293076, Rtriaxial=6372005.51267879) 

30@var Ellipsoids.Fisher1968: Ellipsoid(name='Fisher1968', a=6378150, b=6356768.33724438, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367463.65604381, L=10001988.52191361, R1=6371022.77908146, R2=6371021.18903735, R3=6371014.79995035, Rbiaxial=6367468.14345752, Rtriaxial=6372811.30979281) 

31@var Ellipsoids.GEM10C: Ellipsoid(name='GEM10C', a=6378137, b=6356752.31424783, f_=298.2572236, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367449.14582474, L=10001965.7293148, R1=6371008.77141594, R2=6371007.18091936, R3=6371000.79001005, Rbiaxial=6367453.63451765, Rtriaxial=6372797.55596006) 

32@var Ellipsoids.GPES: Ellipsoid(name='GPES', a=6378135, b=6378135, f_=0, f=0, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6378135, L=10018751.02980197, R1=6378135, R2=6378135, R3=6378135, Rbiaxial=6378135, Rtriaxial=6378135) 

33@var Ellipsoids.GRS67: Ellipsoid(name='GRS67', a=6378160, b=6356774.51609071, f_=298.24716743, f=0.00335292, f2=0.0033642, n=0.00167928, e=0.08182057, e2=0.00669461, e21=0.99330539, e22=0.00673973, e32=0.00335854, A=6367471.74706533, L=10002001.2312605, R1=6371031.50536357, R2=6371029.91475409, R3=6371023.52339015, Rbiaxial=6367476.23607738, Rtriaxial=6372820.3568989) 

34@var Ellipsoids.GRS80: Ellipsoid(name='GRS80', a=6378137, b=6356752.31414035, f_=298.2572221, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367449.14577104, L=10001965.72923046, R1=6371008.77138012, R2=6371007.18088351, R3=6371000.78997414, Rbiaxial=6367453.634464, Rtriaxial=6372797.55593326) 

35@var Ellipsoids.Helmert1906: Ellipsoid(name='Helmert1906', a=6378200, b=6356818.16962789, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367513.57227074, L=10002066.93013953, R1=6371072.7232093, R2=6371071.13315272, R3=6371064.74401563, Rbiaxial=6367518.05971963, Rtriaxial=6372861.26794141) 

36@var Ellipsoids.IAU76: Ellipsoid(name='IAU76', a=6378140, b=6356755.28815753, f_=298.257, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181922, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367452.13278844, L=10001970.4212264, R1=6371011.76271918, R2=6371010.17221946, R3=6371003.78129754, Rbiaxial=6367456.6214902, Rtriaxial=6372800.54945074) 

37@var Ellipsoids.IERS1989: Ellipsoid(name='IERS1989', a=6378136, b=6356751.30156878, f_=298.257, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181922, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367448.13949125, L=10001964.14856985, R1=6371007.76718959, R2=6371006.17669088, R3=6370999.78577297, Rbiaxial=6367452.62819019, Rtriaxial=6372796.55279934) 

38@var Ellipsoids.IERS1992TOPEX: Ellipsoid(name='IERS1992TOPEX', a=6378136.3, b=6356751.61659215, f_=298.25722356, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367448.44699641, L=10001964.63159783, R1=6371008.07219738, R2=6371006.48170097, R3=6371000.09079236, Rbiaxial=6367452.93568883, Rtriaxial=6372796.85654541) 

39@var Ellipsoids.IERS2003: Ellipsoid(name='IERS2003', a=6378136.6, b=6356751.85797165, f_=298.25642, f=0.00335282, f2=0.0033641, n=0.00167922, e=0.0818193, e2=0.0066944, e21=0.9933056, e22=0.00673951, e32=0.00335844, A=6367448.71771058, L=10001965.05683465, R1=6371008.35265722, R2=6371006.76215217, R3=6371000.37120877, Rbiaxial=6367453.20642742, Rtriaxial=6372797.14192686) 

40@var Ellipsoids.Intl1924: Ellipsoid(name='Intl1924', a=6378388, b=6356911.94612795, f_=297, f=0.003367, f2=0.00337838, n=0.00168634, e=0.08199189, e2=0.00672267, e21=0.99327733, e22=0.00676817, e32=0.00337267, A=6367654.50005758, L=10002288.29898944, R1=6371229.31537598, R2=6371227.71133444, R3=6371221.26587487, Rbiaxial=6367659.02704315, Rtriaxial=6373025.77129687) 

41@var Ellipsoids.Intl1967: Ellipsoid(name='Intl1967', a=6378157.5, b=6356772.2, f_=298.24961539, f=0.0033529, f2=0.00336418, n=0.00167926, e=0.08182023, e2=0.00669455, e21=0.99330545, e22=0.00673967, e32=0.00335852, A=6367469.33894446, L=10001997.44859308, R1=6371029.06666667, R2=6371027.47608389, R3=6371021.08482752, Rbiaxial=6367473.827881, Rtriaxial=6372817.9027631) 

42@var Ellipsoids.Krassovski1940: Ellipsoid(name='Krassovski1940', a=6378245, b=6356863.01877305, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367558.49687498, L=10002137.49754285, R1=6371117.67292435, R2=6371116.08285656, R3=6371109.69367439, Rbiaxial=6367562.98435553, Rtriaxial=6372906.23027515) 

43@var Ellipsoids.Krassowsky1940: Ellipsoid(name='Krassowsky1940', a=6378245, b=6356863.01877305, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367558.49687498, L=10002137.49754285, R1=6371117.67292435, R2=6371116.08285656, R3=6371109.69367439, Rbiaxial=6367562.98435553, Rtriaxial=6372906.23027515) 

44@var Ellipsoids.Maupertuis1738: Ellipsoid(name='Maupertuis1738', a=6397300, b=6363806.28272251, f_=191, f=0.0052356, f2=0.00526316, n=0.00262467, e=0.10219488, e2=0.01044379, e21=0.98955621, e22=0.01055402, e32=0.00524931, A=6380564.13011837, L=10022566.69846922, R1=6386135.42757417, R2=6386131.54144847, R3=6386115.8862823, Rbiaxial=6380575.11882818, Rtriaxial=6388943.03218495) 

45@var Ellipsoids.Mercury1960: Ellipsoid(name='Mercury1960', a=6378166, b=6356784.28360711, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367479.62923643, L=10002013.61254591, R1=6371038.76120237, R2=6371037.17115427, R3=6371030.78205124, Rbiaxial=6367484.1166614, Rtriaxial=6372827.29640037) 

46@var Ellipsoids.Mercury1968Mod: Ellipsoid(name='Mercury1968Mod', a=6378150, b=6356768.33724438, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367463.65604381, L=10001988.52191361, R1=6371022.77908146, R2=6371021.18903735, R3=6371014.79995035, Rbiaxial=6367468.14345752, Rtriaxial=6372811.30979281) 

47@var Ellipsoids.NWL1965: Ellipsoid(name='NWL1965', a=6378145, b=6356759.76948868, f_=298.25, f=0.00335289, f2=0.00336417, n=0.00167926, e=0.08182018, e2=0.00669454, e21=0.99330546, e22=0.00673966, e32=0.00335851, A=6367456.87366841, L=10001977.86818326, R1=6371016.58982956, R2=6371014.999254, R3=6371008.60802667, Rbiaxial=6367461.36258457, Rtriaxial=6372805.42010473) 

48@var Ellipsoids.OSU86F: Ellipsoid(name='OSU86F', a=6378136.2, b=6356751.51693008, f_=298.2572236, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367448.3471653, L=10001964.47478349, R1=6371007.97231003, R2=6371006.38181364, R3=6370999.99090513, Rbiaxial=6367452.83585765, Rtriaxial=6372796.75662978) 

49@var Ellipsoids.OSU91A: Ellipsoid(name='OSU91A', a=6378136.3, b=6356751.6165948, f_=298.2572236, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367448.44699773, L=10001964.63159991, R1=6371008.07219827, R2=6371006.48170186, R3=6371000.09079324, Rbiaxial=6367452.93569015, Rtriaxial=6372796.85654607) 

50@var Ellipsoids.Plessis1817: Ellipsoid(name='Plessis1817', a=6376523, b=6355862.93325557, f_=308.64, f=0.00324002, f2=0.00325055, n=0.00162264, e=0.08043347, e2=0.00646954, e21=0.99353046, e22=0.00651167, e32=0.00324527, A=6366197.15710739, L=9999999.11003639, R1=6369636.31108519, R2=6369634.82608583, R3=6369628.85999668, Rbiaxial=6366201.34758009, Rtriaxial=6371364.26393357) 

51@var Ellipsoids.PZ90: Ellipsoid(name='PZ90', a=6378136, b=6356751.36174571, f_=298.2578393, f=0.0033528, f2=0.00336408, n=0.00167922, e=0.08181911, e2=0.00669437, e21=0.99330563, e22=0.00673948, e32=0.00335842, A=6367448.16955443, L=10001964.19579298, R1=6371007.78724857, R2=6371006.1967588, R3=6370999.80587691, Rbiaxial=6367452.65822809, Rtriaxial=6372796.56780569) 

52@var Ellipsoids.SGS85: Ellipsoid(name='SGS85', a=6378136, b=6356751.30156878, f_=298.257, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181922, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367448.13949125, L=10001964.14856985, R1=6371007.76718959, R2=6371006.17669087, R3=6370999.78577297, Rbiaxial=6367452.62819019, Rtriaxial=6372796.55279934) 

53@var Ellipsoids.SoAmerican1969: Ellipsoid(name='SoAmerican1969', a=6378160, b=6356774.71919531, f_=298.25, f=0.00335289, f2=0.00336417, n=0.00167926, e=0.08182018, e2=0.00669454, e21=0.99330546, e22=0.00673966, e32=0.00335851, A=6367471.84853228, L=10002001.39064442, R1=6371031.5730651, R2=6371029.98248581, R3=6371023.59124344, Rbiaxial=6367476.337459, Rtriaxial=6372820.40754721) 

54@var Ellipsoids.Sphere: Ellipsoid(name='Sphere', a=6371008.771415, b=6371008.771415, f_=0, f=0, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6371008.771415, L=10007557.17611675, R1=6371008.771415, R2=6371008.771415, R3=6371008.771415, Rbiaxial=6371008.771415, Rtriaxial=6371008.771415) 

55@var Ellipsoids.SphereAuthalic: Ellipsoid(name='SphereAuthalic', a=6371000, b=6371000, f_=0, f=0, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6371000, L=10007543.39801029, R1=6371000, R2=6371000, R3=6371000, Rbiaxial=6371000, Rtriaxial=6371000) 

56@var Ellipsoids.SpherePopular: Ellipsoid(name='SpherePopular', a=6378137, b=6378137, f_=0, f=0, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6378137, L=10018754.17139462, R1=6378137, R2=6378137, R3=6378137, Rbiaxial=6378137, Rtriaxial=6378137) 

57@var Ellipsoids.Struve1860: Ellipsoid(name='Struve1860', a=6378298.3, b=6356657.14266956, f_=294.73, f=0.00339294, f2=0.00340449, n=0.00169935, e=0.0823065, e2=0.00677436, e21=0.99322564, e22=0.00682056, e32=0.00339869, A=6367482.31832549, L=10002017.83655714, R1=6371084.58088985, R2=6371082.95208988, R3=6371076.40691418, Rbiaxial=6367486.91530791, Rtriaxial=6372894.90029454) 

58@var Ellipsoids.WGS60: Ellipsoid(name='WGS60', a=6378165, b=6356783.28695944, f_=298.3, f=0.00335233, f2=0.00336361, n=0.00167898, e=0.08181333, e2=0.00669342, e21=0.99330658, e22=0.00673853, e32=0.00335795, A=6367478.63091189, L=10002012.04438139, R1=6371037.76231981, R2=6371036.17227197, R3=6371029.78316994, Rbiaxial=6367483.11833616, Rtriaxial=6372826.29723739) 

59@var Ellipsoids.WGS66: Ellipsoid(name='WGS66', a=6378145, b=6356759.76948868, f_=298.25, f=0.00335289, f2=0.00336417, n=0.00167926, e=0.08182018, e2=0.00669454, e21=0.99330546, e22=0.00673966, e32=0.00335851, A=6367456.87366841, L=10001977.86818326, R1=6371016.58982956, R2=6371014.999254, R3=6371008.60802667, Rbiaxial=6367461.36258457, Rtriaxial=6372805.42010473) 

60@var Ellipsoids.WGS72: Ellipsoid(name='WGS72', a=6378135, b=6356750.52001609, f_=298.26, f=0.00335278, f2=0.00336406, n=0.0016792, e=0.08181881, e2=0.00669432, e21=0.99330568, e22=0.00673943, e32=0.0033584, A=6367447.24862383, L=10001962.74919858, R1=6371006.84000536, R2=6371005.24953886, R3=6370998.8587507, Rbiaxial=6367451.7372317, Rtriaxial=6372795.60727472) 

61@var Ellipsoids.WGS84: Ellipsoid(name='WGS84', a=6378137, b=6356752.31424518, f_=298.25722356, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367449.14582341, L=10001965.72931272, R1=6371008.77141506, R2=6371007.18091847, R3=6371000.79000916, Rbiaxial=6367453.63451633, Rtriaxial=6372797.5559594) 

62@var Ellipsoids.WGS84_NGS: Ellipsoid(name='WGS84_NGS', a=6378137, b=6356752.31414035, f_=298.2572221, f=0.00335281, f2=0.00336409, n=0.00167922, e=0.08181919, e2=0.00669438, e21=0.99330562, e22=0.0067395, e32=0.00335843, A=6367449.14577104, L=10001965.72923046, R1=6371008.77138012, R2=6371007.18088351, R3=6371000.78997414, Rbiaxial=6367453.634464, Rtriaxial=6372797.55593326) 

63''' 

64# make sure int/int division yields float quotient, see .basics 

65from __future__ import division as _; del _ # PYCHOK semicolon 

66 

67from pygeodesy.basics import copysign0, isbool, isint 

68from pygeodesy.constants import EPS, EPS0, EPS02, EPS1, INF, NINF, PI4, PI_2, PI_3, R_M, R_MA, R_FM, \ 

69 _EPSqrt, _EPStol as _TOL, _floatuple as _T, _isfinite, _SQRT2_2, \ 

70 _0_0s, _0_0, _0_5, _1_0, _1_EPS, _2_0, _4_0, _90_0, \ 

71 _0_25, _3_0 # PYCHOK used! 

72from pygeodesy.errors import _AssertionError, IntersectionError, _ValueError, _xattr, _xkwds_not 

73from pygeodesy.fmath import cbrt, cbrt2, fdot, Fhorner, fpowers, hypot, hypot_, \ 

74 hypot1, hypot2, sqrt3, Fsum 

75# from pygeodesy.fsums import Fsum # from .fmath 

76from pygeodesy.interns import NN, _a_, _Airy1830_, _AiryModified_, _b_, _Bessel1841_, _beta_, \ 

77 _Clarke1866_, _Clarke1880IGN_, _DOT_, _f_, _GRS80_, _height_, \ 

78 _Intl1924_, _incompatible_, _invalid_, _Krassovski1940_, \ 

79 _Krassowsky1940_, _lat_, _meridional_, _negative_, _not_finite_, \ 

80 _prime_vertical_, _radius_, _Sphere_, _SPACE_, _vs_, _WGS72_, _WGS84_ 

81# from pygeodesy.lazily import _ALL_LAZY, _ALL_MODS as _MODS # from .named 

82from pygeodesy.named import _lazyNamedEnumItem as _lazy, _name__, _name2__, _NamedEnum, \ 

83 _NamedEnumItem, _NamedTuple, _Pass, _ALL_LAZY, _MODS 

84from pygeodesy.namedTuples import Distance2Tuple, Vector3Tuple, Vector4Tuple 

85from pygeodesy.props import deprecated_Property_RO, Property_RO, property_doc_, \ 

86 deprecated_property_RO, property_RO 

87from pygeodesy.streprs import Fmt, fstr, instr, strs, unstr 

88from pygeodesy.units import Bearing_, Distance, Float, Float_, Height, Lam_, Lat, Meter, \ 

89 Meter2, Meter3, Phi, Phi_, Radius, Radius_, Scalar 

90from pygeodesy.utily import atan1, atan1d, atan2b, degrees90, m2radians, radians2m, sincos2d 

91 

92from math import asinh, atan, atanh, cos, degrees, exp, fabs, radians, sin, sinh, sqrt, tan 

93 

94__all__ = _ALL_LAZY.ellipsoids 

95__version__ = '24.05.21' 

96 

97_f_0_0 = Float(f =_0_0) # zero flattening 

98_f__0_0 = Float(f_=_0_0) # zero inverse flattening 

99# see U{WGS84_f<https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Constants.html>} 

100_f__WGS84 = Float(f_=_1_0 / (1000000000 / 298257223563)) # 298.25722356299997 vs 298.257223563 

101 

102 

103def _aux(lat, inverse, auxLat, clip=90): 

104 '''Return a named auxiliary latitude in C{degrees}. 

105 ''' 

106 return Lat(lat, clip=clip, name=_lat_ if inverse else auxLat.__name__) 

107 

108 

109def _s2_c2(phi): 

110 '''(INTERNAL) Return 2-tuple C{(sin(B{phi})**2, cos(B{phi})**2)}. 

111 ''' 

112 if phi: 

113 s2 = sin(phi)**2 

114 if s2 > EPS: 

115 c2 = _1_0 - s2 

116 if c2 > EPS: 

117 if c2 < EPS1: 

118 return s2, c2 

119 else: 

120 return _1_0, _0_0 # phi == PI_2 

121 return _0_0, _1_0 # phi == 0 

122 

123 

124class a_f2Tuple(_NamedTuple): 

125 '''2-Tuple C{(a, f)} specifying an ellipsoid by I{equatorial} 

126 radius C{a} in C{meter} and scalar I{flattening} C{f}. 

127 

128 @see: Class L{Ellipsoid2}. 

129 ''' 

130 _Names_ = (_a_, _f_) # name 'f' not 'f_' 

131 _Units_ = (_Pass, _Pass) 

132 

133 def __new__(cls, a, f, **name): 

134 '''New L{a_f2Tuple} ellipsoid specification. 

135 

136 @arg a: Equatorial radius (C{scalar} > 0). 

137 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

138 @kwarg name: Optional C{B{name}=NN} (C{str}). 

139 

140 @return: An L{a_f2Tuple}C{(a, f)} instance. 

141 

142 @raise UnitError: Invalid B{C{a}} or B{C{f}}. 

143 

144 @note: C{abs(B{f}) < EPS} is forced to C{B{f}=0}, I{spherical}. 

145 Negative C{B{f}} produces a I{prolate} ellipsoid. 

146 ''' 

147 a = Radius_(a=a) # low=EPS, high=None 

148 f = Float_( f=f, low=None, high=EPS1) 

149 if fabs(f) < EPS: # force spherical 

150 f = _f_0_0 

151 return _NamedTuple.__new__(cls, a, f, **name) 

152 

153 @Property_RO 

154 def b(self): 

155 '''Get the I{polar} radius (C{meter}), M{a * (1 - f)}. 

156 ''' 

157 return a_f2b(self.a, self.f) # PYCHOK .a and .f 

158 

159 def ellipsoid(self, **name): 

160 '''Return an L{Ellipsoid} for this 2-tuple C{(a, f)}. 

161 

162 @kwarg name: Optional C{B{name}=NN} (C{str}). 

163 

164 @raise NameError: A registered C{ellipsoid} with the 

165 same B{C{name}} already exists. 

166 ''' 

167 return Ellipsoid(self.a, f=self.f, name=self._name__(name)) # PYCHOK .a and .f 

168 

169 @Property_RO 

170 def f_(self): 

171 '''Get the I{inverse} flattening (C{scalar}), M{1 / f} == M{a / (a - b)}. 

172 ''' 

173 return f2f_(self.f) # PYCHOK .f 

174 

175 

176class Circle4Tuple(_NamedTuple): 

177 '''4-Tuple C{(radius, height, lat, beta)} of the C{radius} and C{height}, 

178 both conventionally in C{meter} of a parallel I{circle of latitude} at 

179 (geodetic) latitude C{lat} and the I{parametric (or reduced) auxiliary 

180 latitude} C{beta}, both in C{degrees90}. 

181 

182 The C{height} is the (signed) distance along the z-axis between the 

183 parallel and the equator. At near-polar C{lat}s, the C{radius} is C{0}, 

184 the C{height} is the ellipsoid's (signed) polar radius and C{beta} 

185 equals C{lat}. 

186 ''' 

187 _Names_ = (_radius_, _height_, _lat_, _beta_) 

188 _Units_ = ( Radius, Height, Lat, Lat) 

189 

190 

191class Curvature2Tuple(_NamedTuple): 

192 '''2-Tuple C{(meridional, prime_vertical)} of radii of curvature, both in 

193 C{meter}, conventionally. 

194 ''' 

195 _Names_ = (_meridional_, _prime_vertical_) 

196 _Units_ = ( Meter, Meter) 

197 

198 @property_RO 

199 def transverse(self): 

200 '''Get this I{prime_vertical}, aka I{transverse} radius of curvature. 

201 ''' 

202 return self.prime_vertical 

203 

204 

205class Ellipsoid(_NamedEnumItem): 

206 '''Ellipsoid with I{equatorial} and I{polar} radii, I{flattening}, I{inverse 

207 flattening} and other, often used, I{cached} attributes, supporting 

208 I{oblate} and I{prolate} ellipsoidal and I{spherical} earth models. 

209 ''' 

210 _a = 0 # equatorial radius, semi-axis (C{meter}) 

211 _b = 0 # polar radius, semi-axis (C{meter}): a * (f - 1) / f 

212 _f = 0 # (1st) flattening: (a - b) / a 

213 _f_ = 0 # inverse flattening: 1 / f = a / (a - b) 

214 

215 _geodsolve = NN # means, use PYGEODESY_GEODSOLVE 

216 _KsOrder = 8 # Krüger series order (4, 6 or 8) 

217 _rhumbsolve = NN # means, use PYGEODESY_RHUMBSOLVE 

218 

219 def __init__(self, a, b=None, f_=None, f=None, **name): 

220 '''New L{Ellipsoid} from the I{equatorial} radius I{and} either 

221 the I{polar} radius or I{inverse flattening} or I{flattening}. 

222 

223 @arg a: Equatorial radius, semi-axis (C{meter}). 

224 @arg b: Optional polar radius, semi-axis (C{meter}). 

225 @arg f_: Inverse flattening: M{a / (a - b)} (C{float} >>> 1.0). 

226 @arg f: Flattening: M{(a - b) / a} (C{scalar}, near zero for 

227 spherical). 

228 @kwarg name: Optional, unique C{B{name}=NN} (C{str}). 

229 

230 @raise NameError: Ellipsoid with the same B{C{name}} already exists. 

231 

232 @raise ValueError: Invalid B{C{a}}, B{C{b}}, B{C{f_}} or B{C{f}} or 

233 B{C{f_}} and B{C{f}} are incompatible. 

234 

235 @note: M{abs(f_) > 1 / EPS} or M{abs(1 / f_) < EPS} is forced 

236 to M{1 / f_ = 0}, spherical. 

237 ''' 

238 ff_ = f, f_ # assertion below 

239 n = _name__(**name) if name else NN 

240 try: 

241 a = Radius_(a=a) # low=EPS 

242 if not _isfinite(a): 

243 raise ValueError(_SPACE_(_a_, _not_finite_)) 

244 

245 if b: # not in (_0_0, None) 

246 b = Radius_(b=b) # low=EPS 

247 f = a_b2f(a, b) if f is None else Float(f=f) 

248 f_ = f2f_(f) if f_ is None else Float(f_=f_) 

249 elif f is not None: 

250 f = Float(f=f) 

251 b = a_f2b(a, f) 

252 f_ = f2f_(f) if f_ is None else Float(f_=f_) 

253 elif f_: 

254 f_ = Float(f_=f_) 

255 b = a_f_2b(a, f_) # a * (f_ - 1) / f_ 

256 f = f_2f(f_) 

257 else: # only a, spherical 

258 f_ = f = 0 

259 b = a # superfluous 

260 

261 if not f < _1_0: # sanity check, see .ecef.Ecef.__init__ 

262 raise ValueError(_SPACE_(_f_, _invalid_)) 

263 if not _isfinite(b): 

264 raise ValueError(_SPACE_(_b_, _not_finite_)) 

265 

266 if fabs(f) < EPS or a == b or not f_: # spherical 

267 b = a 

268 f = _f_0_0 

269 f_ = _f__0_0 

270 

271 except (TypeError, ValueError) as x: 

272 d = _xkwds_not(None, b=b, f_=f_, f=f) 

273 t = instr(self, a=a, name=n, **d) 

274 raise _ValueError(t, cause=x) 

275 

276 self._a = a 

277 self._b = b 

278 self._f = f 

279 self._f_ = f_ 

280 

281 self._register(Ellipsoids, n) 

282 

283 if f and f_: # see .test/testEllipsoidal.py 

284 d = dict(eps=_TOL) 

285 if None in ff_: # both f_ and f given 

286 d.update(Error=_ValueError, txt=_incompatible_) 

287 self._assert(_1_0 / f, f_=f_, **d) 

288 self._assert(_1_0 / f_, f =f, **d) 

289 self._assert(self.b2_a2, e21=self.e21, eps=EPS) 

290 

291 def __eq__(self, other): 

292 '''Compare this and an other ellipsoid. 

293 

294 @arg other: The other ellipsoid (L{Ellipsoid} or L{Ellipsoid2}). 

295 

296 @return: C{True} if equal, C{False} otherwise. 

297 ''' 

298 return self is other or (isinstance(other, Ellipsoid) and 

299 self.a == other.a and 

300 (self.f == other.f or self.b == other.b)) 

301 

302 def __hash__(self): 

303 return self._hash # memoized 

304 

305 @Property_RO 

306 def a(self): 

307 '''Get the I{equatorial} radius, semi-axis (C{meter}). 

308 ''' 

309 return self._a 

310 

311 equatoradius = a # = Requatorial 

312 

313 @Property_RO 

314 def a2(self): 

315 '''Get the I{equatorial} radius I{squared} (C{meter} I{squared}), M{a**2}. 

316 ''' 

317 return Meter2(a2=self.a**2) 

318 

319 @Property_RO 

320 def a2_(self): 

321 '''Get the inverse of the I{equatorial} radius I{squared} (C{meter} I{squared}), M{1 / a**2}. 

322 ''' 

323 return Float(a2_=_1_0 / self.a2) 

324 

325 @Property_RO 

326 def a_b(self): 

327 '''Get the ratio I{equatorial} over I{polar} radius (C{float}), M{a / b} == M{1 / (1 - f)}. 

328 ''' 

329 return Float(a_b=self.a / self.b if self.f else _1_0) 

330 

331 @Property_RO 

332 def a2_b(self): 

333 '''Get the I{polar} meridional (or polar) radius of curvature (C{meter}), M{a**2 / b}. 

334 

335 @see: U{Radii of Curvature 

336 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>} 

337 and U{Moritz, H. (1980), Geodetic Reference System 1980 

338 <https://WikiPedia.org/wiki/Earth_radius#cite_note-Moritz-2>}. 

339 

340 @note: Symbol C{c} is used by IUGG and IERS for the U{polar radius of curvature 

341 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}, see L{c2} 

342 and L{R2} or L{Rauthalic}. 

343 ''' 

344 return Radius(a2_b=self.a2 / self.b if self.f else self.a) # = rocPolar 

345 

346 @Property_RO 

347 def a2_b2(self): 

348 '''Get the ratio I{equatorial} over I{polar} radius I{squared} (C{float}), 

349 M{(a / b)**2} == M{1 / (1 - e**2)} == M{1 / (1 - e2)} == M{1 / e21}. 

350 ''' 

351 return Float(a2_b2=self.a_b**2 if self.f else _1_0) 

352 

353 @Property_RO 

354 def a_f(self): 

355 '''Get the I{equatorial} radius and I{flattening} (L{a_f2Tuple}), see method C{toEllipsoid2}. 

356 ''' 

357 return a_f2Tuple(self.a, self.f, name=self.name) 

358 

359 @Property_RO 

360 def A(self): 

361 '''Get the UTM I{meridional (or rectifying)} radius (C{meter}). 

362 

363 @see: I{Meridian arc unit} U{Q<https://StudyLib.net/doc/7443565/>}. 

364 ''' 

365 A, n = self.a, self.n 

366 if n: 

367 d = (n + _1_0) * 1048576 / A 

368 if d: # use 6 n**2 terms, half-way between the _KsOrder's 4, 6, 8 

369 # <https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html> 

370 # <https://GeographicLib.SourceForge.io/C++/doc/transversemercator.html> and 

371 # <https://www.MyGeodesy.id.AU/documents/Karney-Krueger%20equations.pdf> (3) 

372 # A *= fhorner(n**2, 1048576, 262144, 16384, 4096, 1600, 784, 441) / 1048576) / (1 + n) 

373 A = Radius(A=Fhorner(n**2, 1048576, 262144, 16384, 4096, 1600, 784, 441).fover(d)) 

374 return A 

375 

376 @Property_RO 

377 def _albersCyl(self): 

378 '''(INTERNAL) Helper for C{auxAuthalic}. 

379 ''' 

380 return _MODS.albers.AlbersEqualAreaCylindrical(datum=self, name=self.name) 

381 

382 @Property_RO 

383 def AlphaKs(self): 

384 '''Get the I{Krüger} U{Alpha series coefficients<https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>} (C{KsOrder}C{-tuple}). 

385 ''' 

386 return self._Kseries( # XXX int/int quotients may require from __future__ import division as _; del _ # PYCHOK semicolon 

387 # n n**2 n**3 n**4 n**5 n**6 n**7 n**8 

388 _T(1/2, -2/3, 5/16, 41/180, -127/288, 7891/37800, 72161/387072, -18975107/50803200), 

389 _T(13/48, -3/5, 557/1440, 281/630, -1983433/1935360, 13769/28800, 148003883/174182400), # PYCHOK unaligned 

390 _T(61/240, -103/140, 15061/26880, 167603/181440, -67102379/29030400, 79682431/79833600), # PYCHOK unaligned 

391 _T(49561/161280, -179/168, 6601661/7257600, 97445/49896, -40176129013/7664025600), # PYCHOK unaligned 

392 _T(34729/80640, -3418889/1995840, 14644087/9123840, 2605413599/622702080), # PYCHOK unaligned 

393 _T(212378941/319334400, -30705481/10378368, 175214326799/58118860800), # PYCHOK unaligned 

394 _T(1522256789/1383782400, -16759934899/3113510400), # PYCHOK unaligned 

395 _T(1424729850961/743921418240)) # PYCHOK unaligned 

396 

397 @Property_RO 

398 def area(self): 

399 '''Get the ellipsoid's surface area (C{meter} I{squared}), M{4 * PI * c2}. 

400 

401 @see: Properties L{areax}, L{c2} and L{R2} and functions 

402 L{ellipsoidalExact.areaOf} and L{ellipsoidalKarney.areaOf}. 

403 ''' 

404 return Meter2(area=self.c2 * PI4) 

405 

406 @Property_RO 

407 def areax(self): 

408 '''Get the ellipsoid's surface area (C{meter} I{squared}), M{4 * PI * c2x}, more 

409 accurate for very I{oblate} ellipsoids. 

410 

411 @see: Properties L{area}, L{c2x} and L{R2x}, class L{GeodesicExact} and 

412 functions L{ellipsoidalExact.areaOf} and L{ellipsoidalKarney.areaOf}. 

413 ''' 

414 return Meter2(areax=self.c2x * PI4) 

415 

416 def _assert(self, val, eps=_TOL, f0=_0_0, Error=_AssertionError, txt=NN, **name_value): 

417 '''(INTERNAL) Assert a C{name=value} vs C{val}. 

418 ''' 

419 for n, v in name_value.items(): 

420 if fabs(v - val) > eps: # PYCHOK no cover 

421 t = (v, _vs_, val) 

422 t = _SPACE_.join(strs(t, prec=12, fmt=Fmt.g)) 

423 t = Fmt.EQUAL(self._DOT_(n), t) 

424 raise Error(t, txt=txt or Fmt.exceeds_eps(eps)) 

425 return Float(v if self.f else f0, name=n) 

426 raise Error(unstr(self._DOT_(self._assert.__name__), val, 

427 eps=eps, f0=f0, **name_value)) 

428 

429 def auxAuthalic(self, lat, inverse=False): 

430 '''Compute the I{authalic} auxiliary latitude or the I{inverse} thereof. 

431 

432 @arg lat: The geodetic (or I{authalic}) latitude (C{degrees90}). 

433 @kwarg inverse: If C{True}, B{C{lat}} is the I{authalic} and 

434 return the geodetic latitude (C{bool}). 

435 

436 @return: The I{authalic} (or geodetic) latitude in C{degrees90}. 

437 

438 @see: U{Inverse-/AuthalicLatitude<https://GeographicLib.SourceForge.io/ 

439 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Authalic latitude 

440 <https://WikiPedia.org/wiki/Latitude#Authalic_latitude>}, and 

441 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, p 16. 

442 ''' 

443 if self.f: 

444 f = self._albersCyl._tanf if inverse else self._albersCyl._txif # PYCHOK attr 

445 lat = atan1d(f(tan(Phi_(lat)))) # PYCHOK attr 

446 return _aux(lat, inverse, Ellipsoid.auxAuthalic) 

447 

448 def auxConformal(self, lat, inverse=False): 

449 '''Compute the I{conformal} auxiliary latitude or the I{inverse} thereof. 

450 

451 @arg lat: The geodetic (or I{conformal}) latitude (C{degrees90}). 

452 @kwarg inverse: If C{True}, B{C{lat}} is the I{conformal} and 

453 return the geodetic latitude (C{bool}). 

454 

455 @return: The I{conformal} (or geodetic) latitude in C{degrees90}. 

456 

457 @see: U{Inverse-/ConformalLatitude<https://GeographicLib.SourceForge.io/ 

458 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Conformal latitude 

459 <https://WikiPedia.org/wiki/Latitude#Conformal_latitude>}, and 

460 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 15-16. 

461 ''' 

462 if self.f: 

463 f = self.es_tauf if inverse else self.es_taupf # PYCHOK attr 

464 lat = atan1d(f(tan(Phi_(lat)))) # PYCHOK attr 

465 return _aux(lat, inverse, Ellipsoid.auxConformal) 

466 

467 def auxGeocentric(self, lat, inverse=False): 

468 '''Compute the I{geocentric} auxiliary latitude or the I{inverse} thereof. 

469 

470 @arg lat: The geodetic (or I{geocentric}) latitude (C{degrees90}). 

471 @kwarg inverse: If C{True}, B{C{lat}} is the geocentric and 

472 return the I{geocentric} latitude (C{bool}). 

473 

474 @return: The I{geocentric} (or geodetic) latitude in C{degrees90}. 

475 

476 @see: U{Inverse-/GeocentricLatitude<https://GeographicLib.SourceForge.io/ 

477 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Geocentric latitude 

478 <https://WikiPedia.org/wiki/Latitude#Geocentric_latitude>}, and 

479 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 17-18. 

480 ''' 

481 if self.f: 

482 f = self.a2_b2 if inverse else self.b2_a2 

483 lat = atan1d(f * tan(Phi_(lat))) 

484 return _aux(lat, inverse, Ellipsoid.auxGeocentric) 

485 

486 def auxIsometric(self, lat, inverse=False): 

487 '''Compute the I{isometric} auxiliary latitude or the I{inverse} thereof. 

488 

489 @arg lat: The geodetic (or I{isometric}) latitude (C{degrees}). 

490 @kwarg inverse: If C{True}, B{C{lat}} is the I{isometric} and 

491 return the geodetic latitude (C{bool}). 

492 

493 @return: The I{isometric} (or geodetic) latitude in C{degrees}. 

494 

495 @note: The I{isometric} latitude for geodetic C{+/-90} is far 

496 outside the C{[-90..+90]} range but the inverse 

497 thereof is the original geodetic latitude. 

498 

499 @see: U{Inverse-/IsometricLatitude<https://GeographicLib.SourceForge.io/ 

500 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Isometric latitude 

501 <https://WikiPedia.org/wiki/Latitude#Isometric_latitude>}, and 

502 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 15-16. 

503 ''' 

504 if self.f: 

505 r = Phi_(lat, clip=0) 

506 lat = degrees(atan1(self.es_tauf(sinh(r))) if inverse else 

507 asinh(self.es_taupf(tan(r)))) 

508 # clip=0, since auxIsometric(+/-90) is far outside [-90..+90] 

509 return _aux(lat, inverse, Ellipsoid.auxIsometric, clip=0) 

510 

511 def auxParametric(self, lat, inverse=False): 

512 '''Compute the I{parametric} auxiliary latitude or the I{inverse} thereof. 

513 

514 @arg lat: The geodetic (or I{parametric}) latitude (C{degrees90}). 

515 @kwarg inverse: If C{True}, B{C{lat}} is the I{parametric} and 

516 return the geodetic latitude (C{bool}). 

517 

518 @return: The I{parametric} (or geodetic) latitude in C{degrees90}. 

519 

520 @see: U{Inverse-/ParametricLatitude<https://GeographicLib.SourceForge.io/ 

521 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Parametric latitude 

522 <https://WikiPedia.org/wiki/Latitude#Parametric_(or_reduced)_latitude>}, 

523 and U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, p 18. 

524 ''' 

525 if self.f: 

526 lat = self._beta(Lat(lat), inverse=inverse) 

527 return _aux(lat, inverse, Ellipsoid.auxParametric) 

528 

529 auxReduced = auxParametric # synonymous 

530 

531 def auxRectifying(self, lat, inverse=False): 

532 '''Compute the I{rectifying} auxiliary latitude or the I{inverse} thereof. 

533 

534 @arg lat: The geodetic (or I{rectifying}) latitude (C{degrees90}). 

535 @kwarg inverse: If C{True}, B{C{lat}} is the I{rectifying} and 

536 return the geodetic latitude (C{bool}). 

537 

538 @return: The I{rectifying} (or geodetic) latitude in C{degrees90}. 

539 

540 @see: U{Inverse-/RectifyingLatitude<https://GeographicLib.SourceForge.io/ 

541 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Rectifying latitude 

542 <https://WikiPedia.org/wiki/Latitude#Rectifying_latitude>}, and 

543 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 16-17. 

544 ''' 

545 if self.f: 

546 lat = Lat(lat) 

547 if 0 < fabs(lat) < _90_0: 

548 if inverse: 

549 e = self._elliptic_e22 

550 d = degrees90(e.fEinv(e.cE * lat / _90_0)) 

551 lat = self.auxParametric(d, inverse=True) 

552 else: 

553 lat = _90_0 * self.Llat(lat) / self.L 

554 return _aux(lat, inverse, Ellipsoid.auxRectifying) 

555 

556 @Property_RO 

557 def b(self): 

558 '''Get the I{polar} radius, semi-axis (C{meter}). 

559 ''' 

560 return self._b 

561 

562 polaradius = b # = Rpolar 

563 

564 @Property_RO 

565 def b_a(self): 

566 '''Get the ratio I{polar} over I{equatorial} radius (C{float}), M{b / a == f1 == 1 - f}. 

567 

568 @see: Property L{f1}. 

569 ''' 

570 return self._assert(self.b / self.a, b_a=self.f1, f0=_1_0) 

571 

572 @Property_RO 

573 def b2(self): 

574 '''Get the I{polar} radius I{squared} (C{float}), M{b**2}. 

575 ''' 

576 return Meter2(b2=self.b**2) 

577 

578 @Property_RO 

579 def b2_a(self): 

580 '''Get the I{equatorial} meridional radius of curvature (C{meter}), M{b**2 / a}, see C{rocMeridional}C{(0)}. 

581 

582 @see: U{Radii of Curvature<https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}. 

583 ''' 

584 return Radius(b2_a=self.b2 / self.a if self.f else self.b) 

585 

586 @Property_RO 

587 def b2_a2(self): 

588 '''Get the ratio I{polar} over I{equatorial} radius I{squared} (C{float}), M{(b / a)**2} 

589 == M{(1 - f)**2} == M{1 - e**2} == C{e21}. 

590 ''' 

591 return Float(b2_a2=self.b_a**2 if self.f else _1_0) 

592 

593 def _beta(self, lat, inverse=False): 

594 '''(INTERNAL) Get the I{parametric (or reduced) auxiliary latitude} or inverse thereof. 

595 ''' 

596 s, c = sincos2d(lat) # like Karney's tand(lat) 

597 s *= self.a_b if inverse else self.b_a 

598 return atan1d(s, c) 

599 

600 @Property_RO 

601 def BetaKs(self): 

602 '''Get the I{Krüger} U{Beta series coefficients<https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>} (C{KsOrder}C{-tuple}). 

603 ''' 

604 return self._Kseries( # XXX int/int quotients may require from __future__ import division as _; del _ # PYCHOK semicolon 

605 # n n**2 n**3 n**4 n**5 n**6 n**7 n**8 

606 _T(1/2, -2/3, 37/96, -1/360, -81/512, 96199/604800, -5406467/38707200, 7944359/67737600), 

607 _T(1/48, 1/15, -437/1440, 46/105, -1118711/3870720, 51841/1209600, 24749483/348364800), # PYCHOK unaligned 

608 _T(17/480, -37/840, -209/4480, 5569/90720, 9261899/58060800, -6457463/17740800), # PYCHOK unaligned 

609 _T(4397/161280, -11/504, -830251/7257600, 466511/2494800, 324154477/7664025600), # PYCHOK unaligned 

610 _T(4583/161280, -108847/3991680, -8005831/63866880, 22894433/124540416), # PYCHOK unaligned 

611 _T(20648693/638668800, -16363163/518918400, -2204645983/12915302400), # PYCHOK unaligne 

612 _T(219941297/5535129600, -497323811/12454041600), # PYCHOK unaligned 

613 _T(191773887257/3719607091200)) # PYCHOK unaligned 

614 

615 @deprecated_Property_RO 

616 def c(self): # PYCHOK no cover 

617 '''DEPRECATED, use property C{R2} or C{Rauthalic}.''' 

618 return self.R2 

619 

620 @Property_RO 

621 def c2(self): 

622 '''Get the I{authalic} earth radius I{squared} (C{meter} I{squared}). 

623 

624 @see: Properties L{c2x}, L{area}, L{R2}, L{Rauthalic}, I{Karney's} U{equation (60) 

625 <https://Link.Springer.com/article/10.1007%2Fs00190-012-0578-z>} and C++ U{Ellipsoid.Area 

626 <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Ellipsoid.html>}, 

627 U{Authalic radius<https://WikiPedia.org/wiki/Earth_radius#Authalic_radius>}, U{Surface area 

628 <https://WikiPedia.org/wiki/Ellipsoid>} and U{surface area 

629 <https://www.Numericana.com/answer/geometry.htm#oblate>}. 

630 ''' 

631 return self._c2f(False) 

632 

633 @Property_RO 

634 def c2x(self): 

635 '''Get the I{authalic} earth radius I{squared} (C{meter} I{squared}), more accurate for very I{oblate} 

636 ellipsoids. 

637 

638 @see: Properties L{c2}, L{areax}, L{R2x}, L{Rauthalicx}, class L{GeodesicExact} and I{Karney}'s comments at C++ 

639 attribute U{GeodesicExact._c2<https://GeographicLib.SourceForge.io/C++/doc/GeodesicExact_8cpp_source.html>}. 

640 ''' 

641 return self._c2f(True) 

642 

643 def _c2f(self, c2x): 

644 '''(INTERNAL) Helper for C{.c2} and C{.c2x}. 

645 ''' 

646 f, c2 = self.f, self.b2 

647 if f: 

648 e = self.e 

649 if e > EPS0: 

650 if f > 0: # .isOblate 

651 c2 *= (asinh(sqrt(self.e22abs)) if c2x else atanh(e)) / e 

652 elif f < 0: # .isProlate 

653 c2 *= atan1(e) / e # XXX asin? 

654 c2 = Meter2(c2=(self.a2 + c2) * _0_5) 

655 return c2 

656 

657 def circle4(self, lat): 

658 '''Get the equatorial or a parallel I{circle of latitude}. 

659 

660 @arg lat: Geodetic latitude (C{degrees90}, C{str}). 

661 

662 @return: A L{Circle4Tuple}C{(radius, height, lat, beta)} 

663 instance. 

664 

665 @raise RangeError: Latitude B{C{lat}} outside valid range and 

666 L{pygeodesy.rangerrors} set to C{True}. 

667 

668 @raise TypeError: Invalid B{C{lat}}. 

669 

670 @raise ValueError: Invalid B{C{lat}}. 

671 

672 @see: Definition of U{I{p} and I{z} under B{Parametric (or reduced) latitude} 

673 <https://WikiPedia.org/wiki/Latitude>}, I{Karney's} C++ U{CircleRadius and CircleHeight 

674 <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Ellipsoid.html>} 

675 and method C{Rlat}. 

676 ''' 

677 lat = Lat(lat) 

678 if lat: 

679 b = lat 

680 if fabs(lat) < _90_0: 

681 if self.f: 

682 b = self._beta(lat) 

683 z, r = sincos2d(b) 

684 r *= self.a 

685 z *= self.b 

686 else: # near-polar 

687 r, z = _0_0, copysign0(self.b, lat) 

688 else: # equator 

689 r = self.a 

690 z = lat = b = _0_0 

691 return Circle4Tuple(r, z, lat, b) 

692 

693 def degrees2m(self, deg, lat=0): 

694 '''Convert an angle to the distance along the equator or 

695 along a parallel of (geodetic) latitude. 

696 

697 @arg deg: The angle (C{degrees}). 

698 @kwarg lat: Parallel latitude (C{degrees90}, C{str}). 

699 

700 @return: Distance (C{meter}, same units as the equatorial 

701 and polar radii) or C{0} for near-polar B{C{lat}}. 

702 

703 @raise RangeError: Latitude B{C{lat}} outside valid range and 

704 L{pygeodesy.rangerrors} set to C{True}. 

705 

706 @raise ValueError: Invalid B{C{deg}} or B{C{lat}}. 

707 ''' 

708 return self.radians2m(radians(deg), lat=lat) 

709 

710 def distance2(self, lat0, lon0, lat1, lon1): 

711 '''I{Approximate} the distance and (initial) bearing between 

712 two points based on the U{local, flat earth approximation 

713 <https://www.EdWilliams.org/avform.htm#flat>} aka U{Hubeny 

714 <https://www.OVG.AT/de/vgi/files/pdf/3781/>} formula. 

715 

716 I{Suitable only for distances of several hundred Km or Miles 

717 and only between points not near-polar}. 

718 

719 @arg lat0: From latitude (C{degrees}). 

720 @arg lon0: From longitude (C{degrees}). 

721 @arg lat1: To latitude (C{degrees}). 

722 @arg lon1: To longitude (C{degrees}). 

723 

724 @return: A L{Distance2Tuple}C{(distance, initial)} with C{distance} 

725 in same units as this ellipsoid's axes. 

726 

727 @note: The meridional and prime_vertical radii of curvature are 

728 taken and scaled I{at the initial latitude}, see C{roc2}. 

729 

730 @see: Function L{pygeodesy.flatLocal}/L{pygeodesy.hubeny}. 

731 ''' 

732 phi0 = Phi_(lat0=lat0) 

733 m, n = self.roc2_(phi0, scaled=True) 

734 m *= Phi_(lat1=lat1) - phi0 

735 n *= Lam_(lon1=lon1) - Lam_(lon0=lon0) 

736 return Distance2Tuple(hypot(m, n), atan2b(n, m)) 

737 

738 @Property_RO 

739 def e(self): 

740 '''Get the I{unsigned, (1st) eccentricity} (C{float}), M{sqrt(1 - (b / a)**2))}, see C{a_b2e}. 

741 

742 @see: Property L{es}. 

743 ''' 

744 return Float(e=sqrt(self.e2abs) if self.e2 else _0_0) 

745 

746 @deprecated_Property_RO 

747 def e12(self): # see property ._e12 

748 '''DEPRECATED, use property C{e21}.''' 

749 return self.e21 

750 

751# @Property_RO 

752# def _e12(self): # see property ._elliptic_e12 

753# # (INTERNAL) until e12 above can be replaced with e21. 

754# return self.e2 / (_1_0 - self.e2) # see I{Karney}'s Ellipsoid._e12 = e2 / (1 - e2) 

755 

756 @Property_RO 

757 def e2(self): 

758 '''Get the I{signed, (1st) eccentricity squared} (C{float}), M{f * (2 - f) 

759 == 1 - (b / a)**2}, see C{a_b2e2}. 

760 ''' 

761 return self._assert(a_b2e2(self.a, self.b), e2=f2e2(self.f)) 

762 

763 @Property_RO 

764 def e2abs(self): 

765 '''Get the I{unsigned, (1st) eccentricity squared} (C{float}). 

766 ''' 

767 return fabs(self.e2) 

768 

769 @Property_RO 

770 def e21(self): 

771 '''Get 1 less I{1st eccentricity squared} (C{float}), M{1 - e**2} 

772 == M{1 - e2} == M{(1 - f)**2} == M{b**2 / a**2}, see C{b2_a2}. 

773 ''' 

774 return self._assert((_1_0 - self.f)**2, e21=_1_0 - self.e2, f0=_1_0) 

775 

776# _e2m = e21 # see I{Karney}'s Ellipsoid._e2m = 1 - _e2 

777 _1_e21 = a2_b2 # == M{1 / e21} == M{1 / (1 - e**2)} 

778 

779 @Property_RO 

780 def e22(self): 

781 '''Get the I{signed, 2nd eccentricity squared} (C{float}), M{e2 / (1 - e2) 

782 == e2 / (1 - f)**2 == (a / b)**2 - 1}, see C{a_b2e22}. 

783 ''' 

784 return self._assert(a_b2e22(self.a, self.b), e22=f2e22(self.f)) 

785 

786 @Property_RO 

787 def e22abs(self): 

788 '''Get the I{unsigned, 2nd eccentricity squared} (C{float}). 

789 ''' 

790 return fabs(self.e22) 

791 

792 @Property_RO 

793 def e32(self): 

794 '''Get the I{signed, 3rd eccentricity squared} (C{float}), M{e2 / (2 - e2) 

795 == (a**2 - b**2) / (a**2 + b**2)}, see C{a_b2e32}. 

796 ''' 

797 return self._assert(a_b2e32(self.a, self.b), e32=f2e32(self.f)) 

798 

799 @Property_RO 

800 def e32abs(self): 

801 '''Get the I{unsigned, 3rd eccentricity squared} (C{float}). 

802 ''' 

803 return fabs(self.e32) 

804 

805 @Property_RO 

806 def e4(self): 

807 '''Get the I{unsignd, (1st) eccentricity} to 4th power (C{float}), M{e**4 == e2**2}. 

808 ''' 

809 return Float(e4=self.e2**2 if self.e2 else _0_0) 

810 

811 eccentricity = e # eccentricity 

812# eccentricity2 = e2 # eccentricity squared 

813 eccentricity1st2 = e2 # first eccentricity squared 

814 eccentricity2nd2 = e22 # second eccentricity squared 

815 eccentricity3rd2 = e32 # third eccentricity squared 

816 

817 def ecef(self, Ecef=None): 

818 '''Return U{ECEF<https://WikiPedia.org/wiki/ECEF>} converter. 

819 

820 @kwarg Ecef: ECEF class to use, default L{EcefKarney}. 

821 

822 @return: An ECEF converter for this C{ellipsoid}. 

823 

824 @raise TypeError: Invalid B{C{Ecef}}. 

825 

826 @see: Module L{pygeodesy.ecef}. 

827 ''' 

828 return _MODS.ecef._4Ecef(self, Ecef) 

829 

830 @Property_RO 

831 def _elliptic_e12(self): # see I{Karney}'s Ellipsoid._e12 

832 '''(INTERNAL) Elliptic helper for C{Rhumb}. 

833 ''' 

834 e12 = self.e2 / (self.e2 - _1_0) # NOT DEPRECATED .e12! 

835 return _MODS.elliptic.Elliptic(e12) 

836 

837 @Property_RO 

838 def _elliptic_e22(self): # aka ._elliptic_ep2 

839 '''(INTERNAL) Elliptic helper for C{auxRectifying}, C{L}, C{Llat}. 

840 ''' 

841 return _MODS.elliptic.Elliptic(-self.e22abs) # complex 

842 

843 equatoradius = a # Requatorial 

844 

845 def e2s(self, s): 

846 '''Compute norm M{sqrt(1 - e2 * s**2)}. 

847 

848 @arg s: Sine value (C{scalar}). 

849 

850 @return: Norm (C{float}). 

851 

852 @raise ValueError: Invalid B{C{s}}. 

853 ''' 

854 return sqrt(self.e2s2(s)) if self.e2 else _1_0 

855 

856 def e2s2(self, s): 

857 '''Compute M{1 - e2 * s**2}. 

858 

859 @arg s: Sine value (C{scalar}). 

860 

861 @return: Result (C{float}). 

862 

863 @raise ValueError: Invalid B{C{s}}. 

864 ''' 

865 r = _1_0 

866 if self.e2: 

867 try: 

868 r -= self.e2 * Scalar(s=s)**2 

869 if r < 0: 

870 raise ValueError(_negative_) 

871 except (TypeError, ValueError) as x: 

872 t = self._DOT_(Ellipsoid.e2s2.__name__) 

873 raise _ValueError(t, s, cause=x) 

874 return r 

875 

876 @Property_RO 

877 def es(self): 

878 '''Get the I{signed (1st) eccentricity} (C{float}). 

879 

880 @see: Property L{e}. 

881 ''' 

882 # note, self.e is always non-negative 

883 return Float(es=copysign0(self.e, self.f)) # see .ups 

884 

885 def es_atanh(self, x): 

886 '''Compute M{es * atanh(es * x)} or M{-es * atan(es * x)} 

887 for I{oblate} respectively I{prolate} ellipsoids where 

888 I{es} is the I{signed} (1st) eccentricity. 

889 

890 @raise ValueError: Invalid B{C{x}}. 

891 

892 @see: Function U{Math::eatanhe<https://GeographicLib.SourceForge.io/ 

893 C++/doc/classGeographicLib_1_1Math.html>}. 

894 ''' 

895 return self._es_atanh(Scalar(x=x)) if self.f else _0_0 

896 

897 def _es_atanh(self, x): # see .albers._atanhee, .AuxLat._atanhee 

898 '''(INTERNAL) Helper for .es_atanh, ._es_taupf2 and ._exp_es_atanh. 

899 ''' 

900 es = self.es # signOf(es) == signOf(f) 

901 return es * (atanh(es * x) if es > 0 else # .isOblate 

902 (-atan(es * x) if es < 0 else # .isProlate 

903 _0_0)) # .isSpherical 

904 

905 @Property_RO 

906 def es_c(self): 

907 '''Get M{(1 - f) * exp(es_atanh(1))} (C{float}), M{b_a * exp(es_atanh(1))}. 

908 ''' 

909 return Float(es_c=(self._exp_es_atanh_1 * self.b_a) if self.f else _1_0) 

910 

911 def es_tauf(self, taup): 

912 '''Compute I{Karney}'s U{equations (19), (20) and (21) 

913 <https://ArXiv.org/abs/1002.1417>}. 

914 

915 @see: I{Karney}'s C++ method U{Math::tauf<https://GeographicLib. 

916 SourceForge.io/C++/doc/classGeographicLib_1_1Math.html>} and 

917 and I{Veness}' JavaScript method U{toLatLon<https://www. 

918 Movable-Type.co.UK/scripts/latlong-utm-mgrs.html>}. 

919 ''' 

920 t = Scalar(taup=taup) 

921 if self.f: # .isEllipsoidal 

922 a = fabs(t) 

923 T = t * (self._exp_es_atanh_1 if a > 70 else self._1_e21) 

924 if fabs(T * _EPSqrt) < _2_0: # handles +/- INF and NAN 

925 s = (a * _TOL) if a > _1_0 else _TOL 

926 for T, _, d in self._es_tauf3(t, T): # max 2 

927 if fabs(d) < s: 

928 break 

929 t = Scalar(tauf=T) 

930 return t 

931 

932 def _es_tauf3(self, taup, T, N=9): # in .utm.Utm._toLLEB 

933 '''(INTERNAL) Yield a 3-tuple C{(τi, iteration, delta)} for at most 

934 B{C{N}} Newton iterations, converging rapidly except when C{delta} 

935 toggles on +/-1.12e-16 or +/-4.47e-16, see C{.utm.Utm._toLLEB}. 

936 ''' 

937 e = self._1_e21 

938 _F2_ = Fsum(T).fsum2f_ # τ0 

939 _tf2 = self._es_taupf2 

940 for i in range(1, N + 1): 

941 a, h = _tf2(T) 

942 d = (taup - a) * (e + T**2) / (hypot1(a) * h) 

943 # = (taup - a) / hypot1(a) / ((e + T**2) / h) 

944 T, d = _F2_(d) # τi, (τi - τi-1) 

945 yield T, i, d 

946 

947 def es_taupf(self, tau): 

948 '''Compute I{Karney}'s U{equations (7), (8) and (9) 

949 <https://ArXiv.org/abs/1002.1417>}. 

950 

951 @see: I{Karney}'s C++ method U{Math::taupf<https://GeographicLib. 

952 SourceForge.io/C++/doc/classGeographicLib_1_1Math.html>}. 

953 ''' 

954 t = Scalar(tau=tau) 

955 if self.f: # .isEllipsoidal 

956 t, _ = self._es_taupf2(t) 

957 t = Scalar(taupf=t) 

958 return t 

959 

960 def _es_taupf2(self, tau): 

961 '''(INTERNAL) Return 2-tuple C{(es_taupf(tau), hypot1(tau))}. 

962 ''' 

963 if _isfinite(tau): 

964 h = hypot1(tau) 

965 s = sinh(self._es_atanh(tau / h)) 

966 a = hypot1(s) * tau - h * s 

967 else: 

968 a, h = tau, INF 

969 return a, h 

970 

971 @Property_RO 

972 def _exp_es_atanh_1(self): 

973 '''(INTERNAL) Helper for .es_c and .es_tauf. 

974 ''' 

975 return exp(self._es_atanh(_1_0)) if self.es else _1_0 

976 

977 @Property_RO 

978 def f(self): 

979 '''Get the I{flattening} (C{scalar}), M{(a - b) / a}, C{0} for spherical, negative for prolate. 

980 ''' 

981 return self._f 

982 

983 @Property_RO 

984 def f_(self): 

985 '''Get the I{inverse flattening} (C{scalar}), M{1 / f} == M{a / (a - b)}, C{0} for spherical, see C{a_b2f_}. 

986 ''' 

987 return self._f_ 

988 

989 @Property_RO 

990 def f1(self): 

991 '''Get the I{1 - flattening} (C{float}), M{f1 == 1 - f == b / a}. 

992 

993 @see: Property L{b_a}. 

994 ''' 

995 return Float(f1=_1_0 - self.f) 

996 

997 @Property_RO 

998 def f2(self): 

999 '''Get the I{2nd flattening} (C{float}), M{(a - b) / b == f / (1 - f)}, C{0} for spherical, see C{a_b2f2}. 

1000 ''' 

1001 return self._assert(self.a_b - _1_0, f2=f2f2(self.f)) 

1002 

1003 @deprecated_Property_RO 

1004 def geodesic(self): 

1005 '''DEPRECATED, use property C{geodesicw}.''' 

1006 return self.geodesicw 

1007 

1008 def geodesic_(self, exact=True): 

1009 '''Get the an I{exact} C{Geodesic...} instance for this ellipsoid. 

1010 

1011 @kwarg exact: If C{bool} return L{GeodesicExact}C{(exact=B{exact}, ...)}, 

1012 otherwise a L{Geodesic}, L{GeodesicExact} or L{GeodesicSolve} 

1013 instance for I{this} ellipsoid. 

1014 

1015 @return: The C{exact} geodesic (C{Geodesic...}). 

1016 

1017 @raise TypeError: Invalid B{C{exact}}. 

1018 

1019 @raise ValueError: Incompatible B{C{exact}} ellipsoid. 

1020 ''' 

1021 if isbool(exact): # for consistenccy with C{.rhumb_} 

1022 g = _MODS.geodesicx.GeodesicExact(self, C4order=30 if exact else 24, 

1023 name=self.name) 

1024 else: 

1025 g = exact 

1026 E = _xattr(g, ellipsoid=None) 

1027 if not (E is self and isinstance(g, self._Geodesics)): 

1028 raise _ValueError(exact=g, ellipsoid=E, txt_not_=self.name) 

1029 return g 

1030 

1031 @property_RO 

1032 def _Geodesics(self): 

1033 '''(INTERNAL) Get all C{Geodesic...} classes, I{once}. 

1034 ''' 

1035 Ellipsoid._Geodesics = t = (_MODS.geodesicw._wrapped.Geodesic, # overwrite property_RO 

1036 _MODS.geodesicx.GeodesicExact, 

1037 _MODS.geodsolve.GeodesicSolve) 

1038 return t 

1039 

1040 @property_RO 

1041 def geodesicw(self): 

1042 '''Get this ellipsoid's I{wrapped} U{geodesicw.Geodesic 

1043 <https://GeographicLib.SourceForge.io/Python/doc/code.html>}, provided 

1044 I{Karney}'s U{geographiclib<https://PyPI.org/project/geographiclib>} 

1045 package is installed. 

1046 ''' 

1047 # if not self.isEllipsoidal: 

1048 # raise _IsnotError(_ellipsoidal_, ellipsoid=self) 

1049 return _MODS.geodesicw.Geodesic(self) 

1050 

1051 @property_RO 

1052 def geodesicx(self): 

1053 '''Get this ellipsoid's I{exact} L{GeodesicExact}. 

1054 ''' 

1055 # if not self.isEllipsoidal: 

1056 # raise _IsnotError(_ellipsoidal_, ellipsoid=self) 

1057 return _MODS.geodesicx.GeodesicExact(self, name=self.name) 

1058 

1059 @property 

1060 def geodsolve(self): 

1061 '''Get this ellipsoid's L{GeodesicSolve}, the I{wrapper} around utility 

1062 U{GeodSolve<https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>}, 

1063 provided the path to the C{GeodSolve} executable is specified with env 

1064 variable C{PYGEODESY_GEODSOLVE} or re-/set with this property.. 

1065 ''' 

1066 # if not self.isEllipsoidal: 

1067 # raise _IsnotError(_ellipsoidal_, ellipsoid=self) 

1068 return _MODS.geodsolve.GeodesicSolve(self, path=self._geodsolve, name=self.name) 

1069 

1070 @geodsolve.setter # PYCHOK setter! 

1071 def geodsolve(self, path): 

1072 '''Re-/set the (fully qualified) path to the U{GeodSolve 

1073 <https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>} executable, 

1074 overriding env variable C{PYGEODESY_GEODSOLVE} (C{str}). 

1075 ''' 

1076 self._geodsolve = path 

1077 

1078 def hartzell4(self, pov, los=None): 

1079 '''Compute the intersection of this ellipsoid's surface and a Line-Of-Sight 

1080 from a Point-Of-View in space. 

1081 

1082 @arg pov: Point-Of-View outside this ellipsoid (C{Cartesian}, L{Ecef9Tuple} 

1083 or L{Vector3d}). 

1084 @kwarg los: Line-Of-Sight, I{direction} to this ellipsoid (L{Vector3d}) or 

1085 C{None} to point to this ellipsoid's center. 

1086 

1087 @return: L{Vector4Tuple}C{(x, y, z, h)} with the cartesian coordinates C{x}, 

1088 C{y} and C{z} of the projection on or the intersection with this 

1089 ellipsoid and the I{distance} C{h} from B{C{pov}} to C{(x, y, z)} 

1090 along B{C{los}}, all in C{meter}, conventionally. 

1091 

1092 @raise IntersectionError: Null B{C{pov}} or B{C{los}} vector, or B{C{pov}} 

1093 is inside this ellipsoid or B{C{los}} points 

1094 outside this ellipsoid or points in an opposite 

1095 direction. 

1096 

1097 @raise TypeError: Invalid B{C{pov}} or B{C{los}}. 

1098 

1099 @see: U{I{Satellite Line-of-Sight Intersection with Earth}<https://StephenHartzell. 

1100 Medium.com/satellite-line-of-sight-intersection-with-earth-d786b4a6a9b6>} and 

1101 methods L{Ellipsoid.height4} and L{Triaxial.hartzell4}. 

1102 ''' 

1103 try: 

1104 v, d = _MODS.triaxials._hartzell2(pov, los, self._triaxial) 

1105 except Exception as x: 

1106 raise IntersectionError(pov=pov, los=los, cause=x) 

1107 return Vector4Tuple(v.x, v.y, v.z, d, name__=self.hartzell4) 

1108 

1109 @Property_RO 

1110 def _hash(self): 

1111 return hash((self.a, self.f)) 

1112 

1113 def height4(self, xyz, normal=True): 

1114 '''Compute the projection on and the height of a cartesian above or below 

1115 this ellipsoid's surface. 

1116 

1117 @arg xyz: The cartesian (C{Cartesian}, L{Ecef9Tuple}, L{Vector3d}, 

1118 L{Vector3Tuple} or L{Vector4Tuple}). 

1119 @kwarg normal: If C{True}, the projection is perpendicular to (the nearest 

1120 point on) this ellipsoid's surface, otherwise the C{radial} 

1121 line to this ellipsoid's center (C{bool}). 

1122 

1123 @return: L{Vector4Tuple}C{(x, y, z, h)} with the cartesian coordinates C{x}, 

1124 C{y} and C{z} of the projection on and the height C{h} above or 

1125 below this ellipsoid's surface, all in C{meter}, conventionally. 

1126 

1127 @raise ValueError: Null B{C{xyz}}. 

1128 

1129 @raise TypeError: Non-cartesian B{C{xyz}}. 

1130 

1131 @see: U{Distance to<https://StackOverflow.com/questions/22959698/distance-from-given-point-to-given-ellipse>} 

1132 and U{intersection with<https://MathWorld.wolfram.com/Ellipse-LineIntersection.html>} an ellipse and 

1133 methods L{Ellipsoid.hartzell4} and L{Triaxial.height4}. 

1134 ''' 

1135 v = _MODS.vector3d._otherV3d(xyz=xyz) 

1136 r = v.length 

1137 

1138 a, b, i = self.a, self.b, None 

1139 if r < EPS0: # EPS 

1140 v = v.times(_0_0) 

1141 h = -a 

1142 

1143 elif self.isSpherical: 

1144 v = v.times(a / r) 

1145 h = r - a 

1146 

1147 elif normal: # perpendicular to ellipsoid 

1148 x, y = hypot(v.x, v.y), fabs(v.z) 

1149 if x < EPS0: # PYCHOK no cover 

1150 z = copysign0(b, v.z) 

1151 v = Vector3Tuple(v.x, v.y, z) 

1152 h = y - b # polar 

1153 elif y < EPS0: # PYCHOK no cover 

1154 t = a / r 

1155 v = v.times_(t, t, 0) # force z=0.0 

1156 h = x - a # equatorial 

1157 else: # normal in 1st quadrant 

1158 x, y, i = _normalTo3(x, y, self) 

1159 t, v = v, v.times_(x, x, y) 

1160 h = t.minus(v).length 

1161 

1162 else: # radial to ellipsoid's center 

1163 h = hypot_(a * v.z, b * v.x, b * v.y) 

1164 t = (a * b / h) if h > EPS0 else _0_0 # EPS 

1165 v = v.times(t) 

1166 h = r * (_1_0 - t) 

1167 

1168 return Vector4Tuple(v.x, v.y, v.z, h, iteration=i, name__=self.height4) 

1169 

1170 def _hubeny_2(self, phi2, phi1, lam21, scaled=True, squared=True): 

1171 '''(INTERNAL) like function C{pygeodesy.flatLocal_}/C{pygeodesy.hubeny_}, 

1172 returning the I{angular} distance in C{radians squared} or C{radians} 

1173 ''' 

1174 m, n = self.roc2_((phi2 + phi1) * _0_5, scaled=scaled) 

1175 h, r = (hypot2, self.a2_) if squared else (hypot, _1_0 / self.a) 

1176 return h(m * (phi2 - phi1), n * lam21) * r 

1177 

1178 @Property_RO 

1179 def isEllipsoidal(self): 

1180 '''Is this model I{ellipsoidal} (C{bool})? 

1181 ''' 

1182 return self.f != 0 

1183 

1184 @Property_RO 

1185 def isOblate(self): 

1186 '''Is this ellipsoid I{oblate} (C{bool})? I{Prolate} or 

1187 spherical otherwise. 

1188 ''' 

1189 return self.f > 0 

1190 

1191 @Property_RO 

1192 def isProlate(self): 

1193 '''Is this ellipsoid I{prolate} (C{bool})? I{Oblate} or 

1194 spherical otherwise. 

1195 ''' 

1196 return self.f < 0 

1197 

1198 @Property_RO 

1199 def isSpherical(self): 

1200 '''Is this ellipsoid I{spherical} (C{bool})? 

1201 ''' 

1202 return self.f == 0 

1203 

1204 def _Kseries(self, *AB8Ks): 

1205 '''(INTERNAL) Compute the 4-, 6- or 8-th order I{Krüger} Alpha 

1206 or Beta series coefficients per I{Karney}'s U{equations (35) 

1207 and (36)<https://ArXiv.org/pdf/1002.1417v3.pdf>}. 

1208 

1209 @arg AB8Ks: 8-Tuple of 8-th order I{Krüger} Alpha or Beta series 

1210 coefficient tuples. 

1211 

1212 @return: I{Krüger} series coefficients (L{KsOrder}C{-tuple}). 

1213 

1214 @see: I{Karney}'s 30-th order U{TMseries30 

1215 <https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>}. 

1216 ''' 

1217 k = self.KsOrder 

1218 if self.n: 

1219 ns = fpowers(self.n, k) 

1220 ks = tuple(fdot(AB8Ks[i][:k-i], *ns[i:]) for i in range(k)) 

1221 else: 

1222 ks = _0_0s(k) 

1223 return ks 

1224 

1225 @property_doc_(''' the I{Krüger} series' order (C{int}), see properties C{AlphaKs}, C{BetaKs}.''') 

1226 def KsOrder(self): 

1227 '''Get the I{Krüger} series' order (C{int} 4, 6 or 8). 

1228 ''' 

1229 return self._KsOrder 

1230 

1231 @KsOrder.setter # PYCHOK setter! 

1232 def KsOrder(self, order): 

1233 '''Set the I{Krüger} series' order (C{int} 4, 6 or 8). 

1234 

1235 @raise ValueError: Invalid B{C{order}}. 

1236 ''' 

1237 if not (isint(order) and order in (4, 6, 8)): 

1238 raise _ValueError(order=order) 

1239 if self._KsOrder != order: 

1240 Ellipsoid.AlphaKs._update(self) 

1241 Ellipsoid.BetaKs._update(self) 

1242 self._KsOrder = order 

1243 

1244 @Property_RO 

1245 def L(self): 

1246 '''Get the I{quarter meridian} C{L}, aka the C{polar distance} 

1247 along a meridian between the equator and a pole (C{meter}), 

1248 M{b * Elliptic(-e2 / (1 - e2)).cE} or M{b * PI / 2}. 

1249 ''' 

1250 r = self._elliptic_e22.cE if self.f else PI_2 

1251 return Distance(L=self.b * r) 

1252 

1253 def Llat(self, lat): 

1254 '''Return the I{meridional length}, the distance along a meridian 

1255 between the equator and a (geodetic) latitude, see C{L}. 

1256 

1257 @arg lat: Geodetic latitude (C{degrees90}). 

1258 

1259 @return: The meridional length at B{C{lat}}, negative on southern 

1260 hemisphere (C{meter}). 

1261 ''' 

1262 r = self._elliptic_e22.fEd(self.auxParametric(lat)) if self.f else Phi_(lat) 

1263 return Distance(Llat=self.b * r) 

1264 

1265 Lmeridian = Llat # meridional distance 

1266 

1267 @property_RO 

1268 def _Lpd(self): 

1269 '''Get the I{quarter meridian} per degree (C{meter}), M{self.L / 90}. 

1270 ''' 

1271 return Meter(_Lpd=self.L / _90_0) 

1272 

1273 @property_RO 

1274 def _Lpr(self): 

1275 '''Get the I{quarter meridian} per radian (C{meter}), M{self.L / PI_2}. 

1276 ''' 

1277 return Meter(_Lpr=self.L / PI_2) 

1278 

1279 @deprecated_Property_RO 

1280 def majoradius(self): # PYCHOK no cover 

1281 '''DEPRECATED, use property C{a} or C{Requatorial}.''' 

1282 return self.a 

1283 

1284 def m2degrees(self, distance, lat=0): 

1285 '''Convert a distance to an angle along the equator or 

1286 along a parallel of (geodetic) latitude. 

1287 

1288 @arg distance: Distance (C{meter}). 

1289 @kwarg lat: Parallel latitude (C{degrees90}, C{str}). 

1290 

1291 @return: Angle (C{degrees}) or C{INF} for near-polar B{C{lat}}. 

1292 

1293 @raise RangeError: Latitude B{C{lat}} outside valid range and 

1294 L{pygeodesy.rangerrors} set to C{True}. 

1295 

1296 @raise ValueError: Invalid B{C{distance}} or B{C{lat}}. 

1297 ''' 

1298 return degrees(self.m2radians(distance, lat=lat)) 

1299 

1300 def m2radians(self, distance, lat=0): 

1301 '''Convert a distance to an angle along the equator or 

1302 along a parallel of (geodetic) latitude. 

1303 

1304 @arg distance: Distance (C{meter}). 

1305 @kwarg lat: Parallel latitude (C{degrees90}, C{str}). 

1306 

1307 @return: Angle (C{radians}) or C{INF} for near-polar B{C{lat}}. 

1308 

1309 @raise RangeError: Latitude B{C{lat}} outside valid range and 

1310 L{pygeodesy.rangerrors} set to C{True}. 

1311 

1312 @raise ValueError: Invalid B{C{distance}} or B{C{lat}}. 

1313 ''' 

1314 r = self.circle4(lat).radius if lat else self.a 

1315 return m2radians(distance, radius=r, lat=0) 

1316 

1317 @deprecated_Property_RO 

1318 def minoradius(self): # PYCHOK no cover 

1319 '''DEPRECATED, use property C{b}, C{polaradius} or C{Rpolar}.''' 

1320 return self.b 

1321 

1322 @Property_RO 

1323 def n(self): 

1324 '''Get the I{3rd flattening} (C{float}), M{f / (2 - f) == (a - b) / (a + b)}, see C{a_b2n}. 

1325 ''' 

1326 return self._assert(a_b2n(self.a, self.b), n=f2n(self.f)) 

1327 

1328 flattening = f 

1329 flattening1st = f 

1330 flattening2nd = f2 

1331 flattening3rd = n 

1332 

1333 polaradius = b # Rpolar 

1334 

1335# @Property_RO 

1336# def Q(self): 

1337# '''Get the I{meridian arc unit} C{Q}, the mean, meridional length I{per radian} C({float}). 

1338# 

1339# @note: C{Q * PI / 2} ≈ C{L}, the I{quarter meridian}. 

1340# 

1341# @see: Property C{A} and U{Engsager, K., Poder, K.<https://StudyLib.net/doc/7443565/ 

1342# a-highly-accurate-world-wide-algorithm-for-the-transverse...>}. 

1343# ''' 

1344# n = self.n 

1345# d = (n + _1_0) / self.a 

1346# return Float(Q=Fhorner(n**2, _1_0, _0_25, _1_16th, _0_25).fover(d) if d else self.b) 

1347 

1348# # Moritz, H. <https://Geodesy.Geology.Ohio-State.EDU/course/refpapers/00740128.pdf> 

1349# # Q = (1 - 3/4 * e'2 + 45/64 * e'4 - 175/256 * e'6 + 11025/16384 * e'8) * rocPolar 

1350# # = (4 + e'2 * (-3 + e'2 * (45/16 + e'2 * (-175/64 + e'2 * 11025/4096)))) * rocPolar / 4 

1351# return Fhorner(self.e22, 4, -3, 45 / 16, -175 / 64, 11025 / 4096).fover(4 / self.rocPolar) 

1352 

1353 @deprecated_Property_RO 

1354 def quarteradius(self): # PYCHOK no cover 

1355 '''DEPRECATED, use property C{L} or method C{Llat}.''' 

1356 return self.L 

1357 

1358 @Property_RO 

1359 def R1(self): 

1360 '''Get the I{mean} earth radius per I{IUGG} (C{meter}), M{(2 * a + b) / 3 == a * (1 - f / 3)}. 

1361 

1362 @see: U{Earth radius<https://WikiPedia.org/wiki/Earth_radius>} 

1363 and method C{Rgeometric}. 

1364 ''' 

1365 r = Fsum(self.a, self.a, self.b).fover(_3_0) if self.f else self.a 

1366 return Radius(R1=r) 

1367 

1368 Rmean = R1 

1369 

1370 @Property_RO 

1371 def R2(self): 

1372 '''Get the I{authalic} earth radius (C{meter}), M{sqrt(c2)}. 

1373 

1374 @see: C{R2x}, C{c2}, C{area} and U{Earth radius 

1375 <https://WikiPedia.org/wiki/Earth_radius>}. 

1376 ''' 

1377 return Radius(R2=sqrt(self.c2) if self.f else self.a) 

1378 

1379 Rauthalic = R2 

1380 

1381# @Property_RO 

1382# def R2(self): 

1383# # Moritz, H. <https://Geodesy.Geology.Ohio-State.EDU/course/refpapers/00740128.pdf> 

1384# # R2 = (1 - 2/3 * e'2 + 26/45 * e'4 - 100/189 * e'6 + 7034/14175 * e'8) * rocPolar 

1385# # = (3 + e'2 * (-2 + e'2 * (26/15 + e'2 * (-100/63 + e'2 * 7034/4725)))) * rocPolar / 3 

1386# return Fhorner(self.e22, 3, -2, 26 / 15, -100 / 63, 7034 / 4725).fover(3 / self.rocPolar) 

1387 

1388 @Property_RO 

1389 def R2x(self): 

1390 '''Get the I{authalic} earth radius (C{meter}), M{sqrt(c2x)}. 

1391 

1392 @see: C{R2}, C{c2x} and C{areax}. 

1393 ''' 

1394 return Radius(R2x=sqrt(self.c2x) if self.f else self.a) 

1395 

1396 Rauthalicx = R2x 

1397 

1398 @Property_RO 

1399 def R3(self): 

1400 '''Get the I{volumetric} earth radius (C{meter}), M{(a * a * b)**(1/3)}. 

1401 

1402 @see: U{Earth radius<https://WikiPedia.org/wiki/Earth_radius>} and C{volume}. 

1403 ''' 

1404 r = (cbrt(self.b_a) * self.a) if self.f else self.a 

1405 return Radius(R3=r) 

1406 

1407 Rvolumetric = R3 

1408 

1409 def radians2m(self, rad, lat=0): 

1410 '''Convert an angle to the distance along the equator or 

1411 along a parallel of (geodetic) latitude. 

1412 

1413 @arg rad: The angle (C{radians}). 

1414 @kwarg lat: Parallel latitude (C{degrees90}, C{str}). 

1415 

1416 @return: Distance (C{meter}, same units as the equatorial 

1417 and polar radii) or C{0} for near-polar B{C{lat}}. 

1418 

1419 @raise RangeError: Latitude B{C{lat}} outside valid range and 

1420 L{pygeodesy.rangerrors} set to C{True}. 

1421 

1422 @raise ValueError: Invalid B{C{rad}} or B{C{lat}}. 

1423 ''' 

1424 r = self.circle4(lat).radius if lat else self.a 

1425 return radians2m(rad, radius=r, lat=0) 

1426 

1427 @Property_RO 

1428 def Rbiaxial(self): 

1429 '''Get the I{biaxial, quadratic} mean earth radius (C{meter}), M{sqrt((a**2 + b**2) / 2)}. 

1430 

1431 @see: C{Rtriaxial} 

1432 ''' 

1433 a, b = self.a, self.b 

1434 if b < a: 

1435 b = sqrt(_0_5 + self.b2_a2 * _0_5) * a 

1436 elif b > a: 

1437 b *= sqrt(_0_5 + self.a2_b2 * _0_5) 

1438 return Radius(Rbiaxial=b) 

1439 

1440 Requatorial = a # for consistent naming 

1441 

1442 def Rgeocentric(self, lat): 

1443 '''Compute the I{geocentric} earth radius of (geodetic) latitude. 

1444 

1445 @arg lat: Latitude (C{degrees90}). 

1446 

1447 @return: Geocentric earth radius (C{meter}). 

1448 

1449 @raise ValueError: Invalid B{C{lat}}. 

1450 

1451 @see: U{Geocentric Radius 

1452 <https://WikiPedia.org/wiki/Earth_radius#Geocentric_radius>} 

1453 ''' 

1454 r, a = self.a, Phi_(lat) 

1455 if a and self.f: 

1456 if fabs(a) < PI_2: 

1457 s2, c2 = _s2_c2(a) 

1458 b2_a2_s2 = self.b2_a2 * s2 

1459 # R == sqrt((a2**2 * c2 + b2**2 * s2) / (a2 * c2 + b2 * s2)) 

1460 # == sqrt(a2**2 * (c2 + (b2 / a2)**2 * s2) / (a2 * (c2 + b2 / a2 * s2))) 

1461 # == sqrt(a2 * (c2 + (b2 / a2)**2 * s2) / (c2 + (b2 / a2) * s2)) 

1462 # == a * sqrt((c2 + b2_a2 * b2_a2 * s2) / (c2 + b2_a2 * s2)) 

1463 # == a * sqrt((c2 + b2_a2 * b2_a2_s2) / (c2 + b2_a2_s2)) 

1464 r *= sqrt((c2 + b2_a2_s2 * self.b2_a2) / (c2 + b2_a2_s2)) 

1465 else: 

1466 r = self.b 

1467 return Radius(Rgeocentric=r) 

1468 

1469 @Property_RO 

1470 def Rgeometric(self): 

1471 '''Get the I{geometric} mean earth radius (C{meter}), M{sqrt(a * b)}. 

1472 

1473 @see: C{R1}. 

1474 ''' 

1475 g = sqrt(self.a * self.b) if self.f else self.a 

1476 return Radius(Rgeometric=g) 

1477 

1478 def rhumb_(self, exact=True): 

1479 '''Get the an I{exact} C{Rhumb...} instance for this ellipsoid. 

1480 

1481 @kwarg exact: If C{bool} or C{None} return L{Rhumb}C{(exact=B{exact}, ...)}, 

1482 otherwise a L{Rhumb}, L{RhumbAux} or L{RhumbSolve} instance 

1483 for I{this} ellipsoid. 

1484 

1485 @return: The C{exact} rhumb (C{Rhumb...}). 

1486 

1487 @raise TypeError: Invalid B{C{exact}}. 

1488 

1489 @raise ValueError: Incompatible B{C{exact}} ellipsoid. 

1490 ''' 

1491 if isbool(exact): # use Rhumb for backward compatibility 

1492 r = _MODS.rhumb.ekx.Rhumb(self, exact=exact, name=self.name) 

1493 else: 

1494 r = exact 

1495 E = _xattr(r, ellipsoid=None) 

1496 if not (E is self and isinstance(r, self._Rhumbs)): 

1497 raise _ValueError(exact=r, ellipsosid=E, txt_not_=self.name) 

1498 return r 

1499 

1500 @property_RO 

1501 def rhumbaux(self): 

1502 '''Get this ellipsoid's I{Auxiliary} C{rhumb.RhumbAux}. 

1503 ''' 

1504 # if not self.isEllipsoidal: 

1505 # raise _IsnotError(_ellipsoidal_, ellipsoid=self) 

1506 return _MODS.rhumb.aux_.RhumbAux(self, name=self.name) 

1507 

1508 @property_RO 

1509 def rhumbekx(self): 

1510 '''Get this ellipsoid's I{Elliptic, Krüger} C{rhumb.Rhumb}. 

1511 ''' 

1512 # if not self.isEllipsoidal: 

1513 # raise _IsnotError(_ellipsoidal_, ellipsoid=self) 

1514 return _MODS.rhumb.ekx.Rhumb(self, name=self.name) 

1515 

1516 @property_RO 

1517 def _Rhumbs(self): 

1518 '''(INTERNAL) Get all C{Rhumb...} classes, I{once}. 

1519 ''' 

1520 p = _MODS.rhumb 

1521 Ellipsoid._Rhumbs = t = (p.aux_.RhumbAux, # overwrite property_RO 

1522 p.ekx.Rhumb, p.solve.RhumbSolve) 

1523 return t 

1524 

1525 @property 

1526 def rhumbsolve(self): 

1527 '''Get this ellipsoid's L{RhumbSolve}, the I{wrapper} around utility 

1528 U{RhumbSolve<https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>}, 

1529 provided the path to the C{RhumbSolve} executable is specified with env 

1530 variable C{PYGEODESY_RHUMBSOLVE} or re-/set with this property. 

1531 ''' 

1532 # if not self.isEllipsoidal: 

1533 # raise _IsnotError(_ellipsoidal_, ellipsoid=self) 

1534 return _MODS.rhumb.solve.RhumbSolve(self, path=self._rhumbsolve, name=self.name) 

1535 

1536 @rhumbsolve.setter # PYCHOK setter! 

1537 def rhumbsolve(self, path): 

1538 '''Re-/set the (fully qualified) path to the U{RhumbSolve 

1539 <https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>} executable, 

1540 overriding env variable C{PYGEODESY_RHUMBSOLVE} (C{str}). 

1541 ''' 

1542 self._rhumbsolve = path 

1543 

1544 @deprecated_property_RO 

1545 def rhumbx(self): 

1546 '''DEPRECATED on 2023.11.28, use property C{rhumbekx}. ''' 

1547 return self.rhumbekx 

1548 

1549 def Rlat(self, lat): 

1550 '''I{Approximate} the earth radius of (geodetic) latitude. 

1551 

1552 @arg lat: Latitude (C{degrees90}). 

1553 

1554 @return: Approximate earth radius (C{meter}). 

1555 

1556 @raise RangeError: Latitude B{C{lat}} outside valid range and 

1557 L{pygeodesy.rangerrors} set to C{True}. 

1558 

1559 @raise TypeError: Invalid B{C{lat}}. 

1560 

1561 @raise ValueError: Invalid B{C{lat}}. 

1562 

1563 @note: C{Rlat(B{90})} equals C{Rpolar}. 

1564 

1565 @see: Method C{circle4}. 

1566 ''' 

1567 # r = a - (a - b) * |lat| / 90 

1568 r = self.a 

1569 if self.f and lat: # .isEllipsoidal 

1570 r -= (r - self.b) * fabs(Lat(lat)) / _90_0 

1571 r = Radius(Rlat=r) 

1572 return r 

1573 

1574 Rpolar = b # for consistent naming 

1575 

1576 def roc1_(self, sa, ca=None): 

1577 '''Compute the I{prime-vertical}, I{normal} radius of curvature 

1578 of (geodetic) latitude, I{unscaled}. 

1579 

1580 @arg sa: Sine of the latitude (C{float}, [-1.0..+1.0]). 

1581 @kwarg ca: Optional cosine of the latitude (C{float}, [-1.0..+1.0]) 

1582 to use an alternate formula. 

1583 

1584 @return: The prime-vertical radius of curvature (C{float}). 

1585 

1586 @note: The delta between both formulae with C{Ellipsoids.WGS84} 

1587 is less than 2 nanometer over the entire latitude range. 

1588 

1589 @see: Method L{roc2_} and class L{EcefYou}. 

1590 ''' 

1591 if not self.f: # .isSpherical 

1592 n = self.a 

1593 elif ca is None: 

1594 r = self.e2s2(sa) # see .roc2_ and _EcefBase._forward 

1595 n = sqrt(self.a2 / r) if r > EPS02 else _0_0 

1596 elif ca: # derived from EcefYou.forward 

1597 h = hypot(ca, self.b_a * sa) if sa else fabs(ca) 

1598 n = self.a / h 

1599 elif sa: 

1600 n = self.a2_b / fabs(sa) 

1601 else: 

1602 n = self.a 

1603 return n 

1604 

1605 def roc2(self, lat, scaled=False): 

1606 '''Compute the I{meridional} and I{prime-vertical}, I{normal} 

1607 radii of curvature of (geodetic) latitude. 

1608 

1609 @arg lat: Latitude (C{degrees90}). 

1610 @kwarg scaled: Scale prime_vertical by C{cos(radians(B{lat}))} (C{bool}). 

1611 

1612 @return: An L{Curvature2Tuple}C{(meridional, prime_vertical)} with 

1613 the radii of curvature. 

1614 

1615 @raise ValueError: Invalid B{C{lat}}. 

1616 

1617 @see: Methods L{roc2_} and L{roc1_}, U{Local, flat earth approximation 

1618 <https://www.EdWilliams.org/avform.htm#flat>} and meridional and 

1619 prime vertical U{Radii of Curvature<https://WikiPedia.org/wiki/ 

1620 Earth_radius#Radii_of_curvature>}. 

1621 ''' 

1622 return self.roc2_(Phi_(lat), scaled=scaled) 

1623 

1624 def roc2_(self, phi, scaled=False): 

1625 '''Compute the I{meridional} and I{prime-vertical}, I{normal} radii of 

1626 curvature of (geodetic) latitude. 

1627 

1628 @arg phi: Latitude (C{radians}). 

1629 @kwarg scaled: Scale prime_vertical by C{cos(B{phi})} (C{bool}). 

1630 

1631 @return: An L{Curvature2Tuple}C{(meridional, prime_vertical)} with the 

1632 radii of curvature. 

1633 

1634 @raise ValueError: Invalid B{C{phi}}. 

1635 

1636 @see: Methods L{roc2} and L{roc1_}, property L{rocEquatorial2}, U{Local, 

1637 flat earth approximation<https://www.EdWilliams.org/avform.htm#flat>} 

1638 and the meridional and prime vertical U{Radii of Curvature 

1639 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}. 

1640 ''' 

1641 a = fabs(Phi(phi)) 

1642 if self.f: 

1643 r = self.e2s2(sin(a)) 

1644 if r > EPS02: 

1645 n = self.a / sqrt(r) 

1646 m = n * self.e21 / r # PYCHOK attr 

1647 else: 

1648 m = n = _0_0 # PYCHOK attr 

1649 else: 

1650 m = n = self.a 

1651 if scaled and a: 

1652 n *= cos(a) if a < PI_2 else _0_0 

1653 return Curvature2Tuple(Radius(rocMeridional=m), 

1654 Radius(rocPrimeVertical=n)) 

1655 

1656 def rocBearing(self, lat, bearing): 

1657 '''Compute the I{directional} radius of curvature of (geodetic) 

1658 latitude and compass direction. 

1659 

1660 @arg lat: Latitude (C{degrees90}). 

1661 @arg bearing: Direction (compass C{degrees360}). 

1662 

1663 @return: Directional radius of curvature (C{meter}). 

1664 

1665 @raise RangeError: Latitude B{C{lat}} outside valid range and 

1666 L{pygeodesy.rangerrors} set to C{True}. 

1667 

1668 @raise ValueError: Invalid B{C{lat}} or B{C{bearing}}. 

1669 

1670 @see: U{Radii of Curvature<https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>} 

1671 ''' 

1672 if self.f: 

1673 s2, c2 = _s2_c2(Bearing_(bearing)) 

1674 m, n = self.roc2_(Phi_(lat)) 

1675 if n < m: # == n / (c2 * n / m + s2) 

1676 c2 *= n / m 

1677 elif m < n: # == m / (c2 + s2 * m / n) 

1678 s2 *= m / n 

1679 n = m 

1680 b = n / (c2 + s2) # == 1 / (c2 / m + s2 / n) 

1681 else: 

1682 b = self.b # == self.a 

1683 return Radius(rocBearing=b) 

1684 

1685 @Property_RO 

1686 def rocEquatorial2(self): 

1687 '''Get the I{meridional} and I{prime-vertical}, I{normal} radii of curvature 

1688 at the equator as L{Curvature2Tuple}C{(meridional, prime_vertical)}. 

1689 

1690 @see: Methods L{rocMeridional} and L{rocPrimeVertical}, properties L{b2_a}, 

1691 L{a2_b}, C{rocPolar} and polar and equatorial U{Radii of Curvature 

1692 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}. 

1693 ''' 

1694 return Curvature2Tuple(Radius(rocMeridional0=self.b2_a if self.f else self.a), 

1695 Radius(rocPrimeVertical0=self.a)) 

1696 

1697 def rocGauss(self, lat): 

1698 '''Compute the I{Gaussian} radius of curvature of (geodetic) latitude. 

1699 

1700 @arg lat: Latitude (C{degrees90}). 

1701 

1702 @return: Gaussian radius of curvature (C{meter}). 

1703 

1704 @raise ValueError: Invalid B{C{lat}}. 

1705 

1706 @see: Non-directional U{Radii of Curvature<https://WikiPedia.org/wiki/ 

1707 Earth_radius#Radii_of_curvature>} 

1708 ''' 

1709 # using ... 

1710 # m, n = self.roc2_(Phi_(lat)) 

1711 # return sqrt(m * n) 

1712 # ... requires 1 or 2 sqrt 

1713 g = self.b 

1714 if self.f: 

1715 s2, c2 = _s2_c2(Phi_(lat)) 

1716 g = g / (c2 + self.b2_a2 * s2) 

1717 return Radius(rocGauss=g) 

1718 

1719 def rocMean(self, lat): 

1720 '''Compute the I{mean} radius of curvature of (geodetic) latitude. 

1721 

1722 @arg lat: Latitude (C{degrees90}). 

1723 

1724 @return: Mean radius of curvature (C{meter}). 

1725 

1726 @raise ValueError: Invalid B{C{lat}}. 

1727 

1728 @see: Non-directional U{Radii of Curvature<https://WikiPedia.org/wiki/ 

1729 Earth_radius#Radii_of_curvature>} 

1730 ''' 

1731 if self.f: 

1732 m, n = self.roc2_(Phi_(lat)) 

1733 m *= n * _2_0 / (m + n) # == 2 / (1 / m + 1 / n) 

1734 else: 

1735 m = self.a 

1736 return Radius(rocMean=m) 

1737 

1738 def rocMeridional(self, lat): 

1739 '''Compute the I{meridional} radius of curvature of (geodetic) latitude. 

1740 

1741 @arg lat: Latitude (C{degrees90}). 

1742 

1743 @return: Meridional radius of curvature (C{meter}). 

1744 

1745 @raise ValueError: Invalid B{C{lat}}. 

1746 

1747 @see: Methods L{roc2} and L{roc2_}, U{Local, flat earth approximation 

1748 <https://www.EdWilliams.org/avform.htm#flat>} and U{Radii of 

1749 Curvature<https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}. 

1750 ''' 

1751 return self.roc2_(Phi_(lat)).meridional if lat else \ 

1752 self.rocEquatorial2.meridional 

1753 

1754 rocPolar = a2_b # synonymous 

1755 

1756 def rocPrimeVertical(self, lat): 

1757 '''Compute the I{prime-vertical}, I{normal} radius of curvature of 

1758 (geodetic) latitude, aka the I{transverse} radius of curvature. 

1759 

1760 @arg lat: Latitude (C{degrees90}). 

1761 

1762 @return: Prime-vertical radius of curvature (C{meter}). 

1763 

1764 @raise ValueError: Invalid B{C{lat}}. 

1765 

1766 @see: Methods L{roc2}, L{roc2_} and L{roc1_}, U{Local, flat earth 

1767 approximation<https://www.EdWilliams.org/avform.htm#flat>} and 

1768 U{Radii of Curvature<https://WikiPedia.org/wiki/ 

1769 Earth_radius#Radii_of_curvature>}. 

1770 ''' 

1771 return self.roc2_(Phi_(lat)).prime_vertical if lat else \ 

1772 self.rocEquatorial2.prime_vertical 

1773 

1774 rocTransverse = rocPrimeVertical # synonymous 

1775 

1776 @deprecated_Property_RO 

1777 def Rquadratic(self): # PYCHOK no cover 

1778 '''DEPRECATED, use property C{Rbiaxial} or C{Rtriaxial}.''' 

1779 return self.Rbiaxial 

1780 

1781 @deprecated_Property_RO 

1782 def Rr(self): # PYCHOK no cover 

1783 '''DEPRECATED, use property C{Rrectifying}.''' 

1784 return self.Rrectifying 

1785 

1786 @Property_RO 

1787 def Rrectifying(self): 

1788 '''Get the I{rectifying} earth radius (C{meter}), M{((a**(3/2) + b**(3/2)) / 2)**(2/3)}. 

1789 

1790 @see: U{Earth radius<https://WikiPedia.org/wiki/Earth_radius>}. 

1791 ''' 

1792 r = (cbrt2((_1_0 + sqrt3(self.b_a)) * _0_5) * self.a) if self.f else self.a 

1793 return Radius(Rrectifying=r) 

1794 

1795 @deprecated_Property_RO 

1796 def Rs(self): # PYCHOK no cover 

1797 '''DEPRECATED, use property C{Rgeometric}.''' 

1798 return self.Rgeometric 

1799 

1800 @Property_RO 

1801 def Rtriaxial(self): 

1802 '''Get the I{triaxial, quadratic} mean earth radius (C{meter}), M{sqrt((3 * a**2 + b**2) / 4)}. 

1803 

1804 @see: C{Rbiaxial} 

1805 ''' 

1806 a, b = self.a, self.b 

1807 q = (sqrt((_3_0 + self.b2_a2) * _0_25) * a) if a > b else ( 

1808 (sqrt((_3_0 * self.a2_b2 + _1_0) * _0_25) * b) if a < b else a) 

1809 return Radius(Rtriaxial=q) 

1810 

1811 def toEllipsoid2(self, **name): 

1812 '''Get a copy of this ellipsoid as an L{Ellipsoid2}. 

1813 

1814 @kwarg name: Optional, unique C{B{name}=NN} (C{str}). 

1815 

1816 @see: Property C{a_f}. 

1817 ''' 

1818 return Ellipsoid2(self, None, **name) 

1819 

1820 def toStr(self, prec=8, terse=0, **name): # PYCHOK expected 

1821 '''Return this ellipsoid as a text string. 

1822 

1823 @kwarg prec: Number of decimal digits, unstripped (C{int}). 

1824 @kwarg terse: Limit the number of items (C{int}, 0...18). 

1825 @kwarg name: Optional C{B{name}=NN} (C{str}) or C{None} to 

1826 exclude this ellipsoid's name. 

1827 

1828 @return: This C{Ellipsoid}'s attributes (C{str}). 

1829 ''' 

1830 E = Ellipsoid 

1831 t = E.a, E.b, E.f_, E.f, E.f2, E.n, E.e, E.e2, E.e21, E.e22, E.e32, \ 

1832 E.A, E.L, E.R1, E.R2, E.R3, E.Rbiaxial, E.Rtriaxial 

1833 if terse: 

1834 t = t[:terse] 

1835 n, _ = _name2__(**name) # name=None 

1836 return self._instr(n, prec, props=t) 

1837 

1838 def toTriaxial(self, **name): 

1839 '''Convert this ellipsoid to a L{Triaxial_}. 

1840 

1841 @kwarg name: Optional C{B{name}=NN} (C{str}). 

1842 

1843 @return: A L{Triaxial_} or L{Triaxial} with the C{X} axis 

1844 pointing east and C{Z} pointing north. 

1845 

1846 @see: Method L{Triaxial_.toEllipsoid}. 

1847 ''' 

1848 T = self._triaxial 

1849 return T.copy(**name) if name else T 

1850 

1851 @property_RO 

1852 def _triaxial(self): 

1853 '''(INTERNAL) Get this ellipsoid's un-/ordered C{Triaxial/_}. 

1854 ''' 

1855 a, b, m = self.a, self.b, _MODS.triaxials 

1856 T = m.Triaxial if a > b else m.Triaxial_ 

1857 return T(a, a, b, name=self.name) 

1858 

1859 @Property_RO 

1860 def volume(self): 

1861 '''Get the ellipsoid's I{volume} (C{meter**3}), M{4 / 3 * PI * R3**3}. 

1862 

1863 @see: C{R3}. 

1864 ''' 

1865 return Meter3(volume=self.a2 * self.b * PI_3 * _4_0) 

1866 

1867 

1868class Ellipsoid2(Ellipsoid): 

1869 '''An L{Ellipsoid} specified by I{equatorial} radius and I{flattening}. 

1870 ''' 

1871 def __init__(self, a, f=None, **name): 

1872 '''New L{Ellipsoid2}. 

1873 

1874 @arg a: Equatorial radius, semi-axis (C{meter}) or a previous 

1875 L{Ellipsoid} instance. 

1876 @arg f: Flattening: (C{float} < 1.0, negative for I{prolate}), 

1877 if B{C{a}} is in C{meter}. 

1878 @kwarg name: Optional, unique C{B{name}=NN} (C{str}). 

1879 

1880 @raise NameError: Ellipsoid with that B{C{name}} already exists. 

1881 

1882 @raise ValueError: Invalid B{C{a}} or B{C{f}}. 

1883 

1884 @note: C{abs(B{f}) < EPS} is forced to C{B{f}=0}, I{spherical}. 

1885 Negative C{B{f}} produces a I{prolate} ellipsoid. 

1886 ''' 

1887 if f is None and isinstance(a, Ellipsoid): 

1888 Ellipsoid.__init__(self, a.a, f =a.f, 

1889 b=a.b, f_=a.f_, **name) 

1890 else: 

1891 Ellipsoid.__init__(self, a, f=f, **name) 

1892 

1893 

1894def _spherical_a_b(a, b): 

1895 '''(INTERNAL) C{True} for spherical or invalid C{a} or C{b}. 

1896 ''' 

1897 return a < EPS0 or b < EPS0 or fabs(a - b) < EPS0 

1898 

1899 

1900def _spherical_f(f): 

1901 '''(INTERNAL) C{True} for spherical or invalid C{f}. 

1902 ''' 

1903 return fabs(f) < EPS or f > EPS1 

1904 

1905 

1906def _spherical_f_(f_): 

1907 '''(INTERNAL) C{True} for spherical or invalid C{f_}. 

1908 ''' 

1909 return fabs(f_) < EPS or fabs(f_) > _1_EPS 

1910 

1911 

1912def a_b2e(a, b): 

1913 '''Return C{e}, the I{1st eccentricity} for a given I{equatorial} and I{polar} radius. 

1914 

1915 @arg a: Equatorial radius (C{scalar} > 0). 

1916 @arg b: Polar radius (C{scalar} > 0). 

1917 

1918 @return: The I{unsigned}, (1st) eccentricity (C{float} or C{0}), 

1919 M{sqrt(1 - (b / a)**2)}. 

1920 

1921 @note: The result is always I{non-negative} and C{0} for I{near-spherical} ellipsoids. 

1922 ''' 

1923 return Float(e=sqrt(fabs(a_b2e2(a, b)))) # == sqrt(fabs(a - b) * (a + b)) / a) 

1924 

1925 

1926def a_b2e2(a, b): 

1927 '''Return C{e2}, the I{1st eccentricity squared} for a given I{equatorial} and I{polar} radius. 

1928 

1929 @arg a: Equatorial radius (C{scalar} > 0). 

1930 @arg b: Polar radius (C{scalar} > 0). 

1931 

1932 @return: The I{signed}, (1st) eccentricity I{squared} (C{float} or C{0}), 

1933 M{1 - (b / a)**2}. 

1934 

1935 @note: The result is positive for I{oblate}, negative for I{prolate} 

1936 or C{0} for I{near-spherical} ellipsoids. 

1937 ''' 

1938 return Float(e2=_0_0 if _spherical_a_b(a, b) else ((a - b) * (a + b) / a**2)) 

1939 

1940 

1941def a_b2e22(a, b): 

1942 '''Return C{e22}, the I{2nd eccentricity squared} for a given I{equatorial} and I{polar} radius. 

1943 

1944 @arg a: Equatorial radius (C{scalar} > 0). 

1945 @arg b: Polar radius (C{scalar} > 0). 

1946 

1947 @return: The I{signed}, 2nd eccentricity I{squared} (C{float} or C{0}), 

1948 M{(a / b)**2 - 1}. 

1949 

1950 @note: The result is positive for I{oblate}, negative for I{prolate} 

1951 or C{0} for I{near-spherical} ellipsoids. 

1952 ''' 

1953 return Float(e22=_0_0 if _spherical_a_b(a, b) else ((a - b) * (a + b) / b**2)) 

1954 

1955 

1956def a_b2e32(a, b): 

1957 '''Return C{e32}, the I{3rd eccentricity squared} for a given I{equatorial} and I{polar} radius. 

1958 

1959 @arg a: Equatorial radius (C{scalar} > 0). 

1960 @arg b: Polar radius (C{scalar} > 0). 

1961 

1962 @return: The I{signed}, 3rd eccentricity I{squared} (C{float} or C{0}), 

1963 M{(a**2 - b**2) / (a**2 + b**2)}. 

1964 

1965 @note: The result is positive for I{oblate}, negative for I{prolate} 

1966 or C{0} for I{near-spherical} ellipsoids. 

1967 ''' 

1968 a2, b2 = a**2, b**2 

1969 return Float(e32=_0_0 if _spherical_a_b(a2, b2) else ((a2 - b2) / (a2 + b2))) 

1970 

1971 

1972def a_b2f(a, b): 

1973 '''Return C{f}, the I{flattening} for a given I{equatorial} and I{polar} radius. 

1974 

1975 @arg a: Equatorial radius (C{scalar} > 0). 

1976 @arg b: Polar radius (C{scalar} > 0). 

1977 

1978 @return: The flattening (C{scalar} or C{0}), M{(a - b) / a}. 

1979 

1980 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0} 

1981 for I{near-spherical} ellipsoids. 

1982 ''' 

1983 f = 0 if _spherical_a_b(a, b) else ((a - b) / a) 

1984 return _f_0_0 if _spherical_f(f) else Float(f=f) 

1985 

1986 

1987def a_b2f_(a, b): 

1988 '''Return C{f_}, the I{inverse flattening} for a given I{equatorial} and I{polar} radius. 

1989 

1990 @arg a: Equatorial radius (C{scalar} > 0). 

1991 @arg b: Polar radius (C{scalar} > 0). 

1992 

1993 @return: The inverse flattening (C{scalar} or C{0}), M{a / (a - b)}. 

1994 

1995 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0} 

1996 for I{near-spherical} ellipsoids. 

1997 ''' 

1998 f_ = 0 if _spherical_a_b(a, b) else (a / float(a - b)) 

1999 return _f__0_0 if _spherical_f_(f_) else Float(f_=f_) 

2000 

2001 

2002def a_b2f2(a, b): 

2003 '''Return C{f2}, the I{2nd flattening} for a given I{equatorial} and I{polar} radius. 

2004 

2005 @arg a: Equatorial radius (C{scalar} > 0). 

2006 @arg b: Polar radius (C{scalar} > 0). 

2007 

2008 @return: The I{signed}, 2nd flattening (C{scalar} or C{0}), M{(a - b) / b}. 

2009 

2010 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0} 

2011 for I{near-spherical} ellipsoids. 

2012 ''' 

2013 t = 0 if _spherical_a_b(a, b) else float(a - b) 

2014 return Float(f2=_0_0 if fabs(t) < EPS0 else (t / b)) 

2015 

2016 

2017def a_b2n(a, b): 

2018 '''Return C{n}, the I{3rd flattening} for a given I{equatorial} and I{polar} radius. 

2019 

2020 @arg a: Equatorial radius (C{scalar} > 0). 

2021 @arg b: Polar radius (C{scalar} > 0). 

2022 

2023 @return: The I{signed}, 3rd flattening (C{scalar} or C{0}), M{(a - b) / (a + b)}. 

2024 

2025 @note: The result is positive for I{oblate}, negative for I{prolate} 

2026 or C{0} for I{near-spherical} ellipsoids. 

2027 ''' 

2028 t = 0 if _spherical_a_b(a, b) else float(a - b) 

2029 return Float(n=_0_0 if fabs(t) < EPS0 else (t / (a + b))) 

2030 

2031 

2032def a_f2b(a, f): 

2033 '''Return C{b}, the I{polar} radius for a given I{equatorial} radius and I{flattening}. 

2034 

2035 @arg a: Equatorial radius (C{scalar} > 0). 

2036 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2037 

2038 @return: The polar radius (C{float}), M{a * (1 - f)}. 

2039 ''' 

2040 b = a if _spherical_f(f) else (a * (_1_0 - f)) 

2041 return Radius_(b=a if _spherical_a_b(a, b) else b) 

2042 

2043 

2044def a_f_2b(a, f_): 

2045 '''Return C{b}, the I{polar} radius for a given I{equatorial} radius and I{inverse flattening}. 

2046 

2047 @arg a: Equatorial radius (C{scalar} > 0). 

2048 @arg f_: Inverse flattening (C{scalar} >>> 1). 

2049 

2050 @return: The polar radius (C{float}), M{a * (f_ - 1) / f_}. 

2051 ''' 

2052 b = a if _spherical_f_(f_) else (a * (f_ - _1_0) / f_) 

2053 return Radius_(b=a if _spherical_a_b(a, b) else b) 

2054 

2055 

2056def b_f2a(b, f): 

2057 '''Return C{a}, the I{equatorial} radius for a given I{polar} radius and I{flattening}. 

2058 

2059 @arg b: Polar radius (C{scalar} > 0). 

2060 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2061 

2062 @return: The equatorial radius (C{float}), M{b / (1 - f)}. 

2063 ''' 

2064 t = _1_0 - f 

2065 a = b if fabs(t) < EPS0 else (b / t) 

2066 return Radius_(a=b if _spherical_a_b(a, b) else a) 

2067 

2068 

2069def b_f_2a(b, f_): 

2070 '''Return C{a}, the I{equatorial} radius for a given I{polar} radius and I{inverse flattening}. 

2071 

2072 @arg b: Polar radius (C{scalar} > 0). 

2073 @arg f_: Inverse flattening (C{scalar} >>> 1). 

2074 

2075 @return: The equatorial radius (C{float}), M{b * f_ / (f_ - 1)}. 

2076 ''' 

2077 t = f_ - _1_0 

2078 a = b if _spherical_f_(f_) or fabs(t - f_) < EPS0 \ 

2079 or fabs(t) < EPS0 else (b * f_ / t) 

2080 return Radius_(a=b if _spherical_a_b(a, b) else a) 

2081 

2082 

2083def e2f(e): 

2084 '''Return C{f}, the I{flattening} for a given I{1st eccentricity}. 

2085 

2086 @arg e: The (1st) eccentricity (0 <= C{float} < 1) 

2087 

2088 @return: The flattening (C{scalar} or C{0}). 

2089 

2090 @see: Function L{e22f}. 

2091 ''' 

2092 return e22f(e**2) 

2093 

2094 

2095def e22f(e2): 

2096 '''Return C{f}, the I{flattening} for a given I{1st eccentricity squared}. 

2097 

2098 @arg e2: The (1st) eccentricity I{squared}, I{signed} (L{NINF} < C{float} < 1) 

2099 

2100 @return: The flattening (C{float} or C{0}), M{e2 / (sqrt(e2 - 1) + 1)}. 

2101 ''' 

2102 return Float(f=e2 / (sqrt(_1_0 - e2) + _1_0)) if e2 else _f_0_0 

2103 

2104 

2105def f2e2(f): 

2106 '''Return C{e2}, the I{1st eccentricity squared} for a given I{flattening}. 

2107 

2108 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2109 

2110 @return: The I{signed}, (1st) eccentricity I{squared} (C{float} < 1), 

2111 M{f * (2 - f)}. 

2112 

2113 @note: The result is positive for I{oblate}, negative for I{prolate} 

2114 or C{0} for I{near-spherical} ellipsoids. 

2115 

2116 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/ 

2117 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening 

2118 <https://WikiPedia.org/wiki/Flattening>}. 

2119 ''' 

2120 return Float(e2=_0_0 if _spherical_f(f) else (f * (_2_0 - f))) 

2121 

2122 

2123def f2e22(f): 

2124 '''Return C{e22}, the I{2nd eccentricity squared} for a given I{flattening}. 

2125 

2126 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2127 

2128 @return: The I{signed}, 2nd eccentricity I{squared} (C{float} > -1 or 

2129 C{INF}), M{f * (2 - f) / (1 - f)**2}. 

2130 

2131 @note: The result is positive for I{oblate}, negative for I{prolate} 

2132 or C{0} for near-spherical ellipsoids. 

2133 

2134 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/ 

2135 C++/doc/classGeographicLib_1_1Ellipsoid.html>}. 

2136 ''' 

2137 # e2 / (1 - e2) == f * (2 - f) / (1 - f)**2 

2138 t = (_1_0 - f)**2 

2139 return Float(e22=INF if t < EPS0 else (f2e2(f) / t)) # PYCHOK type 

2140 

2141 

2142def f2e32(f): 

2143 '''Return C{e32}, the I{3rd eccentricity squared} for a given I{flattening}. 

2144 

2145 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2146 

2147 @return: The I{signed}, 3rd eccentricity I{squared} (C{float}), 

2148 M{f * (2 - f) / (1 + (1 - f)**2)}. 

2149 

2150 @note: The result is positive for I{oblate}, negative for I{prolate} 

2151 or C{0} for I{near-spherical} ellipsoids. 

2152 

2153 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/ 

2154 C++/doc/classGeographicLib_1_1Ellipsoid.html>}. 

2155 ''' 

2156 # e2 / (2 - e2) == f * (2 - f) / (1 + (1 - f)**2) 

2157 e2 = f2e2(f) 

2158 return Float(e32=e2 / (_2_0 - e2)) 

2159 

2160 

2161def f_2f(f_): 

2162 '''Return C{f}, the I{flattening} for a given I{inverse flattening}. 

2163 

2164 @arg f_: Inverse flattening (C{scalar} >>> 1). 

2165 

2166 @return: The flattening (C{scalar} or C{0}), M{1 / f_}. 

2167 

2168 @note: The result is positive for I{oblate}, negative for I{prolate} 

2169 or C{0} for I{near-spherical} ellipsoids. 

2170 ''' 

2171 f = 0 if _spherical_f_(f_) else _1_0 / f_ 

2172 return _f_0_0 if _spherical_f(f) else Float(f=f) # PYCHOK type 

2173 

2174 

2175def f2f_(f): 

2176 '''Return C{f_}, the I{inverse flattening} for a given I{flattening}. 

2177 

2178 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2179 

2180 @return: The inverse flattening (C{scalar} or C{0}), M{1 / f}. 

2181 

2182 @note: The result is positive for I{oblate}, negative for I{prolate} 

2183 or C{0} for I{near-spherical} ellipsoids. 

2184 ''' 

2185 f_ = 0 if _spherical_f(f) else _1_0 / f 

2186 return _f__0_0 if _spherical_f_(f_) else Float(f_=f_) # PYCHOK type 

2187 

2188 

2189def f2f2(f): 

2190 '''Return C{f2}, the I{2nd flattening} for a given I{flattening}. 

2191 

2192 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2193 

2194 @return: The I{signed}, 2nd flattening (C{scalar} or C{INF}), M{f / (1 - f)}. 

2195 

2196 @note: The result is positive for I{oblate}, negative for I{prolate} 

2197 or C{0} for I{near-spherical} ellipsoids. 

2198 

2199 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/ 

2200 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening 

2201 <https://WikiPedia.org/wiki/Flattening>}. 

2202 ''' 

2203 t = _1_0 - f 

2204 return Float(f2=_0_0 if _spherical_f(f) else (INF if fabs(t) < EPS 

2205 else (f / t))) # PYCHOK type 

2206 

2207 

2208def f2n(f): 

2209 '''Return C{n}, the I{3rd flattening} for a given I{flattening}. 

2210 

2211 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}). 

2212 

2213 @return: The I{signed}, 3rd flattening (-1 <= C{float} < 1), 

2214 M{f / (2 - f)}. 

2215 

2216 @note: The result is positive for I{oblate}, negative for I{prolate} 

2217 or C{0} for I{near-spherical} ellipsoids. 

2218 

2219 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/ 

2220 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening 

2221 <https://WikiPedia.org/wiki/Flattening>}. 

2222 ''' 

2223 return Float(n=_0_0 if _spherical_f(f) else (f / float(_2_0 - f))) 

2224 

2225 

2226def n2e2(n): 

2227 '''Return C{e2}, the I{1st eccentricity squared} for a given I{3rd flattening}. 

2228 

2229 @arg n: The 3rd flattening (-1 <= C{scalar} < 1). 

2230 

2231 @return: The I{signed}, (1st) eccentricity I{squared} (C{float} or NINF), 

2232 M{4 * n / (1 + n)**2}. 

2233 

2234 @note: The result is positive for I{oblate}, negative for I{prolate} 

2235 or C{0} for I{near-spherical} ellipsoids. 

2236 

2237 @see: U{Flattening<https://WikiPedia.org/wiki/Flattening>}. 

2238 ''' 

2239 t = (n + _1_0)**2 

2240 return Float(e2=_0_0 if fabs(n) < EPS0 else 

2241 (NINF if t < EPS0 else (_4_0 * n / t))) 

2242 

2243 

2244def n2f(n): 

2245 '''Return C{f}, the I{flattening} for a given I{3rd flattening}. 

2246 

2247 @arg n: The 3rd flattening (-1 <= C{scalar} < 1). 

2248 

2249 @return: The flattening (C{scalar} or NINF), M{2 * n / (1 + n)}. 

2250 

2251 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/ 

2252 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening 

2253 <https://WikiPedia.org/wiki/Flattening>}. 

2254 ''' 

2255 t = n + _1_0 

2256 f = 0 if fabs(n) < EPS0 else (NINF if t < EPS0 else (_2_0 * n / t)) 

2257 return _f_0_0 if _spherical_f(f) else Float(f=f) 

2258 

2259 

2260def n2f_(n): 

2261 '''Return C{f_}, the I{inverse flattening} for a given I{3rd flattening}. 

2262 

2263 @arg n: The 3rd flattening (-1 <= C{scalar} < 1). 

2264 

2265 @return: The inverse flattening (C{scalar} or C{0}), M{1 / f}. 

2266 

2267 @see: L{n2f} and L{f2f_}. 

2268 ''' 

2269 return f2f_(n2f(n)) 

2270 

2271 

2272def _normalTo3(px, py, E, eps=EPS): # in .height4 above 

2273 '''(INTERNAL) Nearest point on a 2-D ellipse in 1st quadrant. 

2274 

2275 @see: Functions C{pygeodesy.triaxial._normalTo4} and C{-To5}. 

2276 ''' 

2277 a, b, e0 = E.a, E.b, EPS0 

2278 if min(px, py, a, b) < e0: 

2279 raise _AssertionError(px=px, py=py, a=a, b=b, E=E) 

2280 

2281 a2 = a - b * E.b_a 

2282 b2 = b - a * E.a_b 

2283 tx = ty = _SQRT2_2 

2284 _a, _h = fabs, hypot 

2285 for i in range(16): # max 5 

2286 ex = a2 * tx**3 

2287 ey = b2 * ty**3 

2288 

2289 qx = px - ex 

2290 qy = py - ey 

2291 q = _h(qx, qy) 

2292 if q < e0: # PYCHOK no cover 

2293 break 

2294 r = _h(ex - tx * a, 

2295 ey - ty * b) / q 

2296 

2297 sx, tx = tx, min(_1_0, max(0, (ex + qx * r) / a)) 

2298 sy, ty = ty, min(_1_0, max(0, (ey + qy * r) / b)) 

2299 t = _h(ty, tx) 

2300 if t < e0: # PYCHOK no cover 

2301 break 

2302 tx = tx / t # /= chokes PyChecker 

2303 ty = ty / t 

2304 if _a(sx - tx) < eps and \ 

2305 _a(sy - ty) < eps: 

2306 break 

2307 

2308 tx *= a / px 

2309 ty *= b / py 

2310 return tx, ty, i # x and y as fractions 

2311 

2312 

2313class Ellipsoids(_NamedEnum): 

2314 '''(INTERNAL) L{Ellipsoid} registry, I{must} be a sub-class 

2315 to accommodate the L{_LazyNamedEnumItem} properties. 

2316 ''' 

2317 def _Lazy(self, a, b, f_, **kwds): 

2318 '''(INTERNAL) Instantiate the L{Ellipsoid}. 

2319 ''' 

2320 return Ellipsoid(a, b=b, f_=f_, **kwds) 

2321 

2322Ellipsoids = Ellipsoids(Ellipsoid) # PYCHOK singleton 

2323'''Some pre-defined L{Ellipsoid}s, all I{lazily} instantiated.''' 

2324# <https://www.GNU.org/software/gama/manual/html_node/Supported-ellipsoids.html> 

2325# <https://GSSC.ESA.int/navipedia/index.php/Reference_Frames_in_GNSS> 

2326# <https://kb.OSU.edu/dspace/handle/1811/77986> 

2327# <https://www.IBM.com/docs/en/db2/11.5?topic=systems-supported-spheroids> 

2328# <https://w3.Energistics.org/archive/Epicentre/Epicentre_v3.0/DataModel/LogicalDictionary/StandardValues/ellipsoid.html> 

2329# <https://GitHub.com/locationtech/proj4j/blob/master/src/main/java/org/locationtech/proj4j/datum/Ellipsoid.java> 

2330Ellipsoids._assert( # <https://WikiPedia.org/wiki/Earth_ellipsoid> 

2331 Airy1830 = _lazy(_Airy1830_, *_T(6377563.396, _0_0, 299.3249646)), # b=6356256.909 

2332 AiryModified = _lazy(_AiryModified_, *_T(6377340.189, _0_0, 299.3249646)), # b=6356034.448 

2333# APL4_9 = _lazy('APL4_9', *_T(6378137.0, _0_0, 298.24985392)), # Appl. Phys. Lab. 1965 

2334# ANS = _lazy('ANS', *_T(6378160.0, _0_0, 298.25)), # Australian Nat. Spheroid 

2335# AN_SA96 = _lazy('AN_SA96', *_T(6378160.0, _0_0, 298.24985392)), # Australian Nat. South America 

2336 Australia1966 = _lazy('Australia1966', *_T(6378160.0, _0_0, 298.25)), # b=6356774.7192 

2337 ATS1977 = _lazy('ATS1977', *_T(6378135.0, _0_0, 298.257)), # "Average Terrestrial System" 

2338 Bessel1841 = _lazy(_Bessel1841_, *_T(6377397.155, 6356078.962818, 299.152812797)), 

2339 BesselModified = _lazy('BesselModified', *_T(6377492.018, _0_0, 299.1528128)), 

2340# BesselNamibia = _lazy('BesselNamibia', *_T(6377483.865, _0_0, 299.1528128)), 

2341 CGCS2000 = _lazy('CGCS2000', *_T(R_MA, _0_0, 298.257222101)), # BeiDou Coord System (BDC) 

2342# Clarke1858 = _lazy('Clarke1858', *_T(6378293.639, _0_0, 294.260676369)), 

2343 Clarke1866 = _lazy(_Clarke1866_, *_T(6378206.4, 6356583.8, 294.978698214)), 

2344 Clarke1880 = _lazy('Clarke1880', *_T(6378249.145, 6356514.86954978, 293.465)), 

2345 Clarke1880IGN = _lazy(_Clarke1880IGN_, *_T(6378249.2, 6356515.0, 293.466021294)), 

2346 Clarke1880Mod = _lazy('Clarke1880Mod', *_T(6378249.145, 6356514.96639549, 293.466307656)), # aka Clarke1880Arc 

2347 CPM1799 = _lazy('CPM1799', *_T(6375738.7, 6356671.92557493, 334.39)), # Comm. des Poids et Mesures 

2348 Delambre1810 = _lazy('Delambre1810', *_T(6376428.0, 6355957.92616372, 311.5)), # Belgium 

2349 Engelis1985 = _lazy('Engelis1985', *_T(6378136.05, 6356751.32272154, 298.2566)), 

2350# Everest1830 = _lazy('Everest1830', *_T(6377276.345, _0_0, 300.801699997)), 

2351# Everest1948 = _lazy('Everest1948', *_T(6377304.063, _0_0, 300.801699997)), 

2352# Everest1956 = _lazy('Everest1956', *_T(6377301.243, _0_0, 300.801699997)), 

2353 Everest1969 = _lazy('Everest1969', *_T(6377295.664, 6356094.667915, 300.801699997)), 

2354 Everest1975 = _lazy('Everest1975', *_T(6377299.151, 6356098.14512013, 300.8017255)), 

2355 Fisher1968 = _lazy('Fisher1968', *_T(6378150.0, 6356768.33724438, 298.3)), 

2356# Fisher1968Mod = _lazy('Fisher1968Mod', *_T(6378155.0, _0_0, 298.3)), 

2357 GEM10C = _lazy('GEM10C', *_T(R_MA, 6356752.31424783, 298.2572236)), 

2358 GPES = _lazy('GPES', *_T(6378135.0, 6356750.0, _0_0)), # "Gen. Purpose Earth Spheroid" 

2359 GRS67 = _lazy('GRS67', *_T(6378160.0, _0_0, 298.247167427)), # Lucerne b=6356774.516 

2360# GRS67Truncated = _lazy('GRS67Truncated', *_T(6378160.0, _0_0, 298.25)), 

2361 GRS80 = _lazy(_GRS80_, *_T(R_MA, 6356752.314140347, 298.25722210088)), # IUGG, ITRS, ETRS89 

2362# Hayford1924 = _lazy('Hayford1924', *_T(6378388.0, 6356911.94612795, None)), # aka Intl1924 f_=297 

2363 Helmert1906 = _lazy('Helmert1906', *_T(6378200.0, 6356818.16962789, 298.3)), 

2364# Hough1960 = _lazy('Hough1960', *_T(6378270.0, _0_0, 297.0)), 

2365 IAU76 = _lazy('IAU76', *_T(6378140.0, _0_0, 298.257)), # Int'l Astronomical Union 

2366 IERS1989 = _lazy('IERS1989', *_T(6378136.0, _0_0, 298.257)), # b=6356751.302 

2367 IERS1992TOPEX = _lazy('IERS1992TOPEX', *_T(6378136.3, 6356751.61659215, 298.257223563)), # IERS/TOPEX/Poseidon/McCarthy 

2368 IERS2003 = _lazy('IERS2003', *_T(6378136.6, 6356751.85797165, 298.25642)), 

2369 Intl1924 = _lazy(_Intl1924_, *_T(6378388.0, _0_0, 297.0)), # aka Hayford b=6356911.9462795 

2370 Intl1967 = _lazy('Intl1967', *_T(6378157.5, 6356772.2, 298.24961539)), # New Int'l 

2371 Krassovski1940 = _lazy(_Krassovski1940_, *_T(6378245.0, 6356863.01877305, 298.3)), # spelling 

2372 Krassowsky1940 = _lazy(_Krassowsky1940_, *_T(6378245.0, 6356863.01877305, 298.3)), # spelling 

2373# Kaula = _lazy('Kaula', *_T(6378163.0, _0_0, 298.24)), # Kaula 1961 

2374# Lerch = _lazy('Lerch', *_T(6378139.0, _0_0, 298.257)), # Lerch 1979 

2375 Maupertuis1738 = _lazy('Maupertuis1738', *_T(6397300.0, 6363806.28272251, 191.0)), # France 

2376 Mercury1960 = _lazy('Mercury1960', *_T(6378166.0, 6356784.28360711, 298.3)), 

2377 Mercury1968Mod = _lazy('Mercury1968Mod', *_T(6378150.0, 6356768.33724438, 298.3)), 

2378# MERIT = _lazy('MERIT', *_T(6378137.0, _0_0, 298.257)), # MERIT 1983 

2379# NWL10D = _lazy('NWL10D', *_T(6378135.0, _0_0, 298.26)), # Naval Weapons Lab. 

2380 NWL1965 = _lazy('NWL1965', *_T(6378145.0, 6356759.76948868, 298.25)), # Naval Weapons Lab. 

2381# NWL9D = _lazy('NWL9D', *_T(6378145.0, 6356759.76948868, 298.25)), # NWL1965 

2382 OSU86F = _lazy('OSU86F', *_T(6378136.2, 6356751.51693008, 298.2572236)), 

2383 OSU91A = _lazy('OSU91A', *_T(6378136.3, 6356751.6165948, 298.2572236)), 

2384# Plessis1817 = _lazy('Plessis1817', *_T(6397523.0, 6355863.0, 153.56512242)), # XXX incorrect? 

2385 Plessis1817 = _lazy('Plessis1817', *_T(6376523.0, 6355862.93325557, 308.64)), # XXX IGN France 1972 

2386# Prolate = _lazy('Prolate', *_T(6356752.3, R_MA, _0_0)), 

2387 PZ90 = _lazy('PZ90', *_T(6378136.0, _0_0, 298.257839303)), # GLOSNASS PZ-90 and PZ-90.11 

2388# SEAsia = _lazy('SEAsia', *_T(6378155.0, _0_0, 298.3)), # SouthEast Asia 

2389 SGS85 = _lazy('SGS85', *_T(6378136.0, 6356751.30156878, 298.257)), # Soviet Geodetic System 

2390 SoAmerican1969 = _lazy('SoAmerican1969', *_T(6378160.0, 6356774.71919531, 298.25)), # South American 

2391 Sphere = _lazy(_Sphere_, *_T(R_M, R_M, _0_0)), # pseudo 

2392 SphereAuthalic = _lazy('SphereAuthalic', *_T(R_FM, R_FM, _0_0)), # pseudo 

2393 SpherePopular = _lazy('SpherePopular', *_T(R_MA, R_MA, _0_0)), # EPSG:3857 Spheroid 

2394 Struve1860 = _lazy('Struve1860', *_T(6378298.3, 6356657.14266956, 294.73)), 

2395# Walbeck = _lazy('Walbeck', *_T(6376896.0, _0_0, 302.78)), 

2396# WarOffice = _lazy('WarOffice', *_T(6378300.0, _0_0, 296.0)), 

2397 WGS60 = _lazy('WGS60', *_T(6378165.0, 6356783.28695944, 298.3)), 

2398 WGS66 = _lazy('WGS66', *_T(6378145.0, 6356759.76948868, 298.25)), 

2399 WGS72 = _lazy(_WGS72_, *_T(6378135.0, _0_0, 298.26)), # b=6356750.52 

2400 WGS84 = _lazy(_WGS84_, *_T(R_MA, _0_0, _f__WGS84)), # GPS b=6356752.3142451793 

2401# U{NOAA/NOS/NGS/inverse<https://GitHub.com/noaa-ngs/inverse/blob/main/invers3d.f>} 

2402 WGS84_NGS = _lazy('WGS84_NGS', *_T(R_MA, _0_0, 298.257222100882711243162836600094)) 

2403) 

2404 

2405_EWGS84 = Ellipsoids.WGS84 # (INTERNAL) shared 

2406 

2407if __name__ == '__main__': 

2408 

2409 from pygeodesy.interns import _COMMA_, _NL_, _NLATvar_ 

2410 from pygeodesy import nameof, printf 

2411 

2412 for E in (_EWGS84, Ellipsoids.GRS80, # NAD83, 

2413 Ellipsoids.Sphere, Ellipsoids.SpherePopular, 

2414 Ellipsoid(_EWGS84.b, _EWGS84.a, name='_Prolate')): 

2415 e = f2n(E.f) - E.n 

2416 printf('# %s: %s', _DOT_('Ellipsoids', E.name), E.toStr(prec=10), nl=1) 

2417 printf('# e=%s, f_=%s, f=%s, n=%s (%s)', fstr(E.e, prec=13, fmt=Fmt.e), 

2418 fstr(E.f_, prec=13, fmt=Fmt.e), 

2419 fstr(E.f, prec=13, fmt=Fmt.e), 

2420 fstr(E.n, prec=13, fmt=Fmt.e), 

2421 fstr(e, prec=9, fmt=Fmt.e)) 

2422 printf('# %s %s', Ellipsoid.AlphaKs.name, fstr(E.AlphaKs, prec=20)) 

2423 printf('# %s %s', Ellipsoid.BetaKs.name, fstr(E.BetaKs, prec=20)) 

2424 printf('# %s %s', nameof(Ellipsoid.KsOrder), E.KsOrder) # property 

2425 

2426 # __doc__ of this file, force all into registry 

2427 t = [NN] + Ellipsoids.toRepr(all=True, asorted=True).split(_NL_) 

2428 printf(_NLATvar_.join(i.strip(_COMMA_) for i in t)) 

2429 

2430# % python3 -m pygeodesy.ellipsoids 

2431 

2432# Ellipsoids.WGS84: name='WGS84', a=6378137, b=6356752.3142451793, f_=298.257223563, f=0.0033528107, f2=0.0033640898, n=0.0016792204, e=0.0818191908, e2=0.00669438, e21=0.99330562, e22=0.0067394967, e32=0.0033584313, A=6367449.1458234144, L=10001965.7293127235, R1=6371008.7714150595, R2=6371007.1809184738, R3=6371000.7900091587, Rbiaxial=6367453.6345163295, Rtriaxial=6372797.5559594007 

2433# e=8.1819190842622e-02, f_=2.98257223563e+02, f=3.3528106647475e-03, n=1.6792203863837e-03 (0.0e+00) 

2434# AlphaKs 0.00083773182062446994, 0.00000076085277735725, 0.00000000119764550324, 0.00000000000242917068, 0.00000000000000571182, 0.0000000000000000148, 0.00000000000000000004, 0.0 

2435# BetaKs 0.00083773216405794875, 0.0000000590587015222, 0.00000000016734826653, 0.00000000000021647981, 0.00000000000000037879, 0.00000000000000000072, 0.0, 0.0 

2436# KsOrder 8 

2437 

2438# Ellipsoids.GRS80: name='GRS80', a=6378137, b=6356752.3141403468, f_=298.2572221009, f=0.0033528107, f2=0.0033640898, n=0.0016792204, e=0.081819191, e2=0.00669438, e21=0.99330562, e22=0.0067394968, e32=0.0033584313, A=6367449.1457710434, L=10001965.7292304561, R1=6371008.7713801153, R2=6371007.1808835147, R3=6371000.7899741363, Rbiaxial=6367453.6344640013, Rtriaxial=6372797.5559332585 

2439# e=8.1819191042833e-02, f_=2.9825722210088e+02, f=3.3528106811837e-03, n=1.6792203946295e-03 (0.0e+00) 

2440# AlphaKs 0.00083773182472890429, 0.00000076085278481561, 0.00000000119764552086, 0.00000000000242917073, 0.00000000000000571182, 0.0000000000000000148, 0.00000000000000000004, 0.0 

2441# BetaKs 0.0008377321681623882, 0.00000005905870210374, 0.000000000167348269, 0.00000000000021647982, 0.00000000000000037879, 0.00000000000000000072, 0.0, 0.0 

2442# KsOrder 8 

2443 

2444# Ellipsoids.Sphere: name='Sphere', a=6371008.7714149999, b=6371008.7714149999, f_=0, f=0, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6371008.7714149999, L=10007557.1761167478, R1=6371008.7714149999, R2=6371008.7714149999, R3=6371008.7714149999, Rbiaxial=6371008.7714149999, Rtriaxial=6371008.7714149999 

2445# e=0.0e+00, f_=0.0e+00, f=0.0e+00, n=0.0e+00 (0.0e+00) 

2446# AlphaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0 

2447# BetaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0 

2448# KsOrder 8 

2449 

2450# Ellipsoids.SpherePopular: name='SpherePopular', a=6378137, b=6378137, f_=0, f=0, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6378137, L=10018754.171394622, R1=6378137, R2=6378137, R3=6378137, Rbiaxial=6378137, Rtriaxial=6378137 

2451# e=0.0e+00, f_=0.0e+00, f=0.0e+00, n=0.0e+00 (0.0e+00) 

2452# AlphaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0 

2453# BetaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0 

2454# KsOrder 8 

2455 

2456# Ellipsoids._Prolate: name='_Prolate', a=6356752.3142451793, b=6378137, f_=-297.257223563, f=-0.0033640898, f2=-0.0033528107, n=-0.0016792204, e=0.0820944379, e2=-0.0067394967, e21=1.0067394967, e22=-0.00669438, e32=-0.0033584313, A=6367449.1458234144, L=10035500.5204500314, R1=6363880.5428301189, R2=6363878.9413582645, R3=6363872.5644020075, Rbiaxial=6367453.6345163295, Rtriaxial=6362105.2243882557 

2457# e=8.2094437949696e-02, f_=-2.97257223563e+02, f=-3.3640898209765e-03, n=-1.6792203863837e-03 (0.0e+00) 

2458# AlphaKs -0.00084149152514366627, 0.00000076653480614871, -0.00000000120934503389, 0.0000000000024576225, -0.00000000000000578863, 0.00000000000000001502, -0.00000000000000000004, 0.0 

2459# BetaKs -0.00084149187224351817, 0.00000005842735196773, -0.0000000001680487236, 0.00000000000021706261, -0.00000000000000038002, 0.00000000000000000073, -0.0, 0.0 

2460# KsOrder 8 

2461 

2462# **) MIT License 

2463# 

2464# Copyright (C) 2016-2024 -- mrJean1 at Gmail -- All Rights Reserved. 

2465# 

2466# Permission is hereby granted, free of charge, to any person obtaining a 

2467# copy of this software and associated documentation files (the "Software"), 

2468# to deal in the Software without restriction, including without limitation 

2469# the rights to use, copy, modify, merge, publish, distribute, sublicense, 

2470# and/or sell copies of the Software, and to permit persons to whom the 

2471# Software is furnished to do so, subject to the following conditions: 

2472# 

2473# The above copyright notice and this permission notice shall be included 

2474# in all copies or substantial portions of the Software. 

2475# 

2476# THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS 

2477# OR IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY, 

2478# FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL 

2479# THE AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR 

2480# OTHER LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, 

2481# ARISING FROM, OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR 

2482# OTHER DEALINGS IN THE SOFTWARE.