Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jrasc..70..185d&link_type=abstract
Journal of the Royal Astronomical Society of Canada, vol. 70, Aug. 1976, p. 185-192.
Astronomy and Astrophysics
Astronomy
Microwave Emission, Microwave Spectra, Solar Flux Density, Solar Radio Bursts, Solar Activity Effects, Solar Cycles, Sunspots
Scientific paper
The basic, slowly varying, and burst components of the absolute solar radio flux in the microwave region have been examined for the decaying phase (1970-1974) of the solar cycle. Results obtained from this analysis are: (1) the spectra of the basic (B) and the slowly varying (S) component have been found to depend on sunspot activity; (2) the peak of the S-component spectra has been found to occur within the frequency range 2695-4995 MHz; (3) the rates of occurrence of microwave bursts at different frequencies follow similar variations during the period under investigation, whereas these variations are not well correlated with that of the S-component; and (4) the variation of the total energy output in bursts also does not correlate well with that of the S-component flux.
Chattopadhyay Tanuka
Das Gupta M. K.
Sarkar Sanat K.
No associations
LandOfFree
Some studies on the spectra of the different components of the absolute solar microwave flux does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Some studies on the spectra of the different components of the absolute solar microwave flux, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some studies on the spectra of the different components of the absolute solar microwave flux will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1873086