Solar flare effects on 164 kHz LF wave propagation over Tashkent-Patiala path

Details Solar flare effects on 164 kHz LF wave propagation over Tashkent-Patiala path Solar flare effects on 164 kHz LF wave propagation over Tashkent-Patiala path

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ijrsp..18...48s&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 18, April 1989, p. 48-51.

Physics

Space Physics

Low Frequencies, Plasma Temperature, Solar Activity Effects, Solar Flares, Solar X-Rays, Wave Propagation, Diurnal Variations, Histograms, India

Scientific paper

Different types of sudden field anomalies (SFAs) are observed on 164 kHz long wave propagation from Tashkent to Patiala during a solar flare. Type 1 variations occur mostly from June to October, whereas Types II and III occur from November to May. The SFAs are more frequent during winter and equinoxes as compared to summer. The large X-ray flux enhancements in wavelength bands 0.5-3 A and 1-8 A are required for Types I and III effects to occur as compared to Type II effects and the same holds good for hardness factor. There seems to be no correlation with peak time plasma temperature of the X-ray emitting regions.

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