Fine structure of a very bright active region at a wavelength of 2.8 CM

Details Fine structure of a very bright active region at a wavelength of 2.8 CM Fine structure of a very bright active region at a wavelength of 2.8 CM

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...37..395f&link_type=abstract

Solar Physics, vol. 37, Aug. 1974, p. 395-402. Consiglio Nazionale delle Ricerche

Physics

5

Brightness Temperature, Fine Structure, Microwave Emission, Solar Radio Emission, H Alpha Line, Photosphere, Solar Activity, Solar Granulation, Solar Magnetic Field, Solar Temperature

Scientific paper

The radio structure of the active region McMath 11976 has been investigated with an east-west resolution of 16'' at a wavelength of 2.8 cm. Six bright components were found with angular sizes of the order of 20''. From the position measure of these components in two following days the heights above the solar photosphere are determined. Their positions are compared with the H-alpha and magnetic structure of the active region. The derived brightness temperatures reach unusual values, up to six million K for the brightest component.

Affiliated with

Also associated with

No associations

Rating

Fine structure of a very bright active region at a wavelength of 2.8 CM 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 Fine structure of a very bright active region at a wavelength of 2.8 CM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fine structure of a very bright active region at a wavelength of 2.8 CM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1465502