Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.209..297p&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 209, no. 2, p. 297-306
Astronomy and Astrophysics
Astrophysics
6
Phase Deviation, Signal Analysis, Solar Flares, Solar X-Rays, Very Low Frequencies, Absorption Cross Sections, Anomalies, Emission Spectra, Solar Position
Scientific paper
Sudden phase anomalies (SPA's) observed in the phase of Galactic Background Radiation (GBR) 16 kHz VLF signals during the years 1977 to 1983 have been analyzed in the light of their associated solar X-ray fluxes in the 0.5-4 A and 1-8 A bands. An attempt has been made to investigate the solar zenith angle (Chi) dependence of the integrated solar X-ray flux for producing SPA's. It is deduced from the observations for Chi less than 81 deg that the phase deviation increases linearly as a whole with increasing solar X-ray fluxes in these two bands. The threshold X-ray flux needed to produce a detectable SPA effect has been estimated to be 1.6 x 10-4 erg/sq cm/s and 1.8 x 10-3 erg/sq cm/s in the 0.5-4 A and 1-8 A bands, respectively. For both bands the average cross section for all atmospheric constituents at a height of 70 km is almost equal to the absorption cross section for the 3 A X-ray emission.
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