pyart.correct.ptoa_to_sf#

pyart.correct.ptoa_to_sf(ptoa, pulse_width, wavelen, antenna_gain, coeff_band=1.2)[source]#

Converts the sun power at the top of the atmosphere (in dBm) into solar flux.

Parameters:

  • ptoa (float) – sun power at the top of the amosphere. It already takes into account the correction for antenna polarization

  • pulse_width (float) – pulse width [s]

  • wavelen (float) – radar wavelength [m]

  • antenna_gain (float) – the antenna gain [dB]

  • coeff_band (float) – multiplicative coefficient applied to the inverse of the pulse width to get the effective bandwidth

Returns:

s0 (float) – solar flux [10e-22 W/(m2 Hz)]

References

Altube P., J. Bech, O. Argemi, T. Rigo, 2015: Quality Control of Antenna Alignment and Receiver Calibration Using the Sun: Adaptation to Midrange Weather Radar Observations at Low Elevation Angles