High-resolution microwave spectra of solar bursts

Details High-resolution microwave spectra of solar bursts High-resolution microwave spectra of solar bursts

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..351s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 120, no. 2, 1989, p. 351-368.

Physics

48

Microwave Spectra, Solar Flares, Solar Radio Bursts, Brightness Temperature, Gyrofrequency, High Resolution, Synchrotron Radiation

Scientific paper

A phenomenological and statistical study of flares observed in total power with the frequency-agile interferometer at the Owens Valley Radio Observatory during several months of high solar activity in 1981 is reported. Roughly 80 percent of the events have a complex spectrum consisting of more than one spectral component, implying that the microwave radiation of a burst usually does not come from a single homogeneous source. The presence of more than one component can lead to significant errors when data with low spectral resolution are used to determine the low-side spectral index. The low-frequency slope of a single spectra component is often steeper than expected, and the peak frequency stays nearly constant throughout a microwave event.

Affiliated with

Also associated with

No associations

Rating

High-resolution microwave spectra of solar bursts 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 High-resolution microwave spectra of solar bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-resolution microwave spectra of solar bursts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1827144