Ionospheric E region and E — F1 valley as indicators of solar radiant fluxes in the 10 30 nm wavelength region

Details Ionospheric E region and E — F1 valley as indicators of solar radiant fluxes in the 10 30 nm wavelength region Ionospheric E region and E — F1 valley as indicators of solar radiant fluxes in the 10 30 nm wavelength region

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..838n&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 10, pp.838-840

Physics

1

Scientific paper

To estimate the solar radiant flux by an indirect route in the spectrum region from 10 to 30 nm, which is difficult for direct measurement, we propose to use the data on the electron density in the E region maximum and E-F1 valley. Taken from empirical models, the data on these parameters were correlated with theoretical calculations. It is shown that at wavelengths of from 10 to 30 nm the solar radiant flux is about 2.5 times greater than that measured from the AE- E satellite. The results are used to correct the model spectra of extreme UV radiation.

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