SRF
- class typhon.physics.units.SRF(f, W)[source]
- Respresents a spectral response function - TODO: representation of uncertainties - __init__(f, W)[source]
- Initialise SRF object. - You can either initialise an SRF from scratch, or use the classmethod fromArtsXML to read it from a file. - A toy example on initiating it from scratch: - >>> from typhon.physics.units.common import ureg >>> from typhon.physics.units.em import SRF >>> srf = SRF(ureg.Quantity(numpy.array([200, 200.1, 200.2, 200.3, 200.4, 200.5]), 'GHz'), numpy.array([0, 0.5, 1, 1, 0.5, 0])) >>> R_300 = srf.blackbody_radiance(ureg.Quantity(300, 'K')) >>> print(R_300) [ 3.63716781e-15] watt / hertz / meter ** 2 / steradian >>> print(R_300.to("K", "radiance", srf=srf)) [ 300.] kelvin - You can also pass in other spectroscopic units (wavenumber, wavelength) that will be converted internally to frequency: - >>> srf = SRF(ureg.Quantity(numpy.array([10.8, 10.9, 11.0, 11.1, 11.2, 11.3]), 'um'), numpy.array([0, 0.5, 1, 1, 0.5, 0])) >>> R_300 = srf.blackbody_radiance(ureg.Quantity(numpy.atleast_1d(250), 'K')) >>> print(R_300) [ 1.61922509e-12] watt / hertz / meter ** 2 / steradian >>> print(R_300.to("cm * mW / m**2 / sr", "radiance")) [ 48.54314703] centimeter * milliwatt / meter ** 2 / steradian >>> print(R_300.to("K", "radiance", srf=srf)) [ 300.] kelvin - Parameters:
- f (ndarray) – Array of frequencies. Can be either a pure ndarray, which will be assumed to be in Hz, or a ureg quantity. 
- W (ndarray) – Array of associated weights. 
 
 
 - Methods - __init__(f, W)- Initialise SRF object. - as_dataarray(coordinate)- Return xarray.DataArray object. - blackbody_radiance(T[, spectral])- Calculate integrated radiance for blackbody at temperature T - centroid()- Calculate centre frequency - Convert channel radiance to brightness temperature - estimate_band_coefficients([sat, instr, ch, ...])- Estimate band coefficients for fast/explicit BT calculations - fromArtsXML(sat, instr, ch)- Read SRF from ArtsXML files. - fromRTTOV(sat, instr, ch)- Read SRF from RTTOV format files. - integrate_radiances(f, L[, spectral])- From a spectrum of radiances and a SRF, calculate channel (spectral) radiance - Construct lookup table radiance <-> BT - shift(amount)- Get new SRF, shifted by <amount> - Attributes - L_to_T- T_lookup_table- frequency- lookup_table- wavelength- wavenumber