Read hs and p2l Files
This set of functions reads the netcdf files _hs.nc and _p2l.nc produced by WW3.
It contains four functions read_WWNC, read_WWNCf, read_hs and read_p2l:
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read_WWNC (file_path, time_vect, lon1, lat1): Read netcdf _hs.nc file and return a matrix with dimension lon x lat of significant height of wind and swell waves in meters. -
read_WWNCf (file_path, time_vect, lon1, lat1): Read netcdf _p2l.nc file and return latitude, longitude, frequenc, p2l data which is the base 10 logarithm of power specral density of equivalent surface pressure and the units of p2l. -
read_hs (file_path, time_vect, lon1, lat1): Read netcdf significant wave height (_hs.nc) file and return latitude, longitude, frequenc, hs data. Uses xarray. -
read_p2l (file_path, time_vect, lon1, lat1): Read netcdf _p2l.nc file and return latitude, longitude, frequenc, p2l data the units of p2l. Uses xarray.
read_WWNC(file_path, time_vect, lon1, lat1)
Read netcdf _hs.nc file and return a matrix with dimension lon x lat of significant height of wind and swell waves in meters.
Examples:
>>> file_path = '../data/ftp.ifremer.fr/ifremer/ww3/HINDCAST/SISMO/GLOBAL05_2006_REF102040/data/WW3-GLOB-30M_200609_hs.nc'
>>> year = 2006
>>> month = 9
>>> day = 4
>>> hour = 12
>>> lon1 = []
>>> lat1 = []
>>> time_vect = [year, month, day, hour]
>>> A = read_WWNC(file_path, time_vect, [], [])
>>> print(A)
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Source code in wmsan/read_hs_p2l.py
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read_WWNCf(file_path, time_vect, lon1, lat1)
Read netcdf _p2l.nc file and return latitude, longitude, frequenc, p2l data which is the base 10 logarithm of power specral density of equivalent surface pressure and the units of p2l.
Examples:
>>> file_path = '../data/ftp.ifremer.fr/ifremer/ww3/HINDCAST/SISMO/GLOBAL05_2006_REF102040/WW3-GLOB-30M_200609_p2l.nc'
>>> year = 2006
>>> month = 9
>>> day = 4
>>> hour = 12
>>> lon1 = []
>>> lat1 = []
>>> time_vect = [year, month, day, hour]
>>> (lat, lon, freq, p2l, unit1) = read_WWNCf(file_path, time_vect, [], [])
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Source code in wmsan/read_hs_p2l.py
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read_hs(file_path, time_vect, lon1=(-180, 180), lat1=(-90, 90))
Read netcdf significant wave height (_hs.nc) file and return latitude, longitude, frequenc, hs data units are m. The output is an xarray of shape (lat, lon)
Examples:
>>> file_path = '../data/ftp.ifremer.fr/ifremer/ww3/HINDCAST/SISMO/GLOBAL05_2006_REF102040/WW3-GLOB-30M_200609_hs.nc'
>>> year = 2006
>>> month = 9
>>> day = 4
>>> hour = 12
>>> lon1 = [-180, 180]
>>> lat1 = [-90, 90]
>>> time_vect = [year, month, day, hour]
>>> hs = read_hs(file_path, time_vect, lon1, lat1)
>>> fig = plt.figure(figsize=(9,6))
>>> ax = plt.axes(projection=ccrs.Robinson())
>>> ax.coastlines()
>>> ax.gridlines()
>>> hs.plot(ax=ax, transform=ccrs.PlateCarree(), cbar_kwargs={'shrink': 0.4})
>>> plt.show()
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Source code in wmsan/read_hs_p2l.py
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read_p2l(file_path, time_vect, lon1=(-180, 180), lat1=(-90, 90))
Read netcdf _p2l.nc file and return latitude, longitude, frequency, p2l data which is the base 10 logarithm of power specral density of equivalent surface pressure and the units of p2l.
Examples:
>>> file_path = '../data/ftp.ifremer.fr/ifremer/ww3/HINDCAST/SISMO/GLOBAL05_2006_REF102040/WW3-GLOB-30M_200609_p2l.nc'
>>> year = 2006
>>> month = 9
>>> day = 4
>>> hour = 12
>>> lon1 = []
>>> lat1 = []
>>> time_vect = [year, month, day, hour]
>>> (lat, lon, freq, p2l, unit1) = read_WWNCf(file_path, time_vect, lon1, lat1)
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Source code in wmsan/read_hs_p2l.py
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