Solar influence on ELF-VLF emission observed at conjugate stations

Details Solar influence on ELF-VLF emission observed at conjugate stations Solar influence on ELF-VLF emission observed at conjugate stations

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jgr....9611455s&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 96, July 1, 1991, p. 11,455-11,460.

Physics

Extremely Low Frequencies, Solar Activity Effects, Vlf Emission Recorders, Conjugate Points, Geomagnetism, Magnetosphere-Ionosphere Coupling

Scientific paper

Characteristics of the long-term variation of daytime (06-16 hours MLT) ELF-VLF emissions at 750 Hz and 2 kHz are examined. The emission intensity shows obvious quasi-periodic fluctations, with periods of 1 day, about 27 days, 1 year, and about 11 years. The diurnal and seasonal variations are strongly dependent on sunlight in the topside ionosphere. The emission intensity is also affected by geomagnetic activity with quasi-periodicities of about 27 days and about 11 years. It is suggested that sunlight in the ionosphere affects the propagation of waves whereas the solar activity affects their generation.

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