Physics
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jatp...47..979m&link_type=abstract
(IUGG, IAGA, USAF, et al., International Symposium on Equatorial Aeronomy, 7th, Hong Kong, Mar. 22-29, 1984) Journal of Atmosphe
Physics
1
Bursts, Field Strength, Solar Flux, Solar X-Rays, Ground Stations, Ionospheric Electron Density, Low Frequencies, Phase Deviation, Temporal Distribution
Scientific paper
A method of detecting the flux of solar X-ray bursts and its time variation from the ground is presented. The flux is detected by means of the phase and field strength variations of LF signals reflected by the low ionosphere. According to theories of radio wave propagation, ionization, and recombination in the ionosphere, the formula for calculating the solar X-ray bursts flux is deduced in the exponential profile of the low ionosphere. A method of determining the parameters involved has been proposed. Comparisons between calculated values of solar X-ray bursts and satellite-measured values in the 0.5-4 A wavelength range show that detection values obtained by this method conform closely with measured results.
Li De-Min
Miao Y. R.
Tu L.-Z.
Yang K.-J.
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