Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources

Details Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...97..173d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 97, May 1985, p. 173-182.

Astronomy and Astrophysics

Astronomy

Radio Sources (Astronomy), Solar Radio Bursts, Type 2 Bursts, Type 3 Bursts, Type 5 Bursts, Very High Frequencies, Brightness, H Alpha Line, Solar Corona, Solar Flares

Scientific paper

A comparison of quiescent type I solar radio sources with concurrent intense impulsive type III, V, and type II sources shows that whereas the type I sources are usually small and stable the type III, V, and II sources are usually large and unstable. The author concludes that the large size and variability of the type III, V, and II radio sources cannot be attributed to instrumental error or ionospheric refraction but must instead reflect the size and variability of the coronal structures on which they arise.

Affiliated with

Also associated with

No associations

Rating

Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources 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 Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1633599