On the complex spatial structure of a gradual microwave burst

Details On the complex spatial structure of a gradual microwave burst On the complex spatial structure of a gradual microwave burst

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..351b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 129, Oct. 1990, p. 351-361.

Astronomy and Astrophysics

Astronomy

4

Microwave Spectra, Solar Radio Bursts, Spatial Distribution, Brightness Temperature, Radio Astronomy, Solar Corona, Solar Flares, Solar Magnetic Field

Scientific paper

By bringing to bear observations obtained by the RATAN-600 telescope at ten different frequencies in the 0.8-31.6 cm wavelength range, as well as time profiles from the Observatory for Solar Radio Astronomy at Tremsdorf, novel conclusions can be arrived at concerning the extended spectral/spatial structure of the gradual burst even of May 13, 1985. Strong evidence emerges for the emission of as little as 24 percent of the microwave flux from this event by an excessive, small-scale burst source, while the remainder of the burst emission has a larger region, encompassing two major components in the source-area of the S-component radiation, as its origin. An analysis is presented of the different components of the burst and S-component radiation.

Affiliated with

Also associated with

No associations

Rating

On the complex spatial structure of a gradual microwave burst 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 On the complex spatial structure of a gradual microwave burst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the complex spatial structure of a gradual microwave burst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1305734