Computer Science – Numerical Analysis
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..257c&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, July 1988, p. 257-263.
Computer Science
Numerical Analysis
Faculae, Solar Cycles, Solar Radio Emission, Sunspots, Extremum Values, Frequency Ranges, Long Term Effects, Low Frequencies, Numerical Analysis
Scientific paper
The systematic change of the quiet sun emission in the course of the solar cycle at all frequencies is studied. Curves are presented which show the solar cycle variation of the basic component at 1000 MHz, 2000 MHz, 3750 MHz, and 9500 MHz as well as the solar cycle variation of the sunspot number and plage index. The B-component spectra in the solar activity maximum and minimum years show that the range over which the B-component varies changes from one solar cycle to the next.
Chattopadhyay Tanuka
Das Tapas Kumar
Das Gupta M. K.
Sarkar Sanat K.
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