The brightness temperatures of solar type III bursts

Details The brightness temperatures of solar type III bursts The brightness temperatures of solar type III bursts

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..369m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 120, no. 2, 1989, p. 369-381.

Physics

22

Brightness Temperature, Solar Wind, Type 3 Bursts, Electron Distribution, Saturation, Solar Corona

Scientific paper

The suggestion is explored that the maximum brightness temperature T(B) of roughly 10 to the 15th K observed for type III solar radio bursts in the solar wind may be attributed to saturation of the processes involved in the plasma emission. The processes leading to fundamental and second harmonic emission saturate when T(B) is about equal to the effective temperature of the Langmuir waves. The expected maximum value of T(B) is estimated for this saturation from the growth rate for the beam instability and from the maximum amplitude of the observed Langmuir turbulence. Agreement with observational values is satisfactory.

Affiliated with

Also associated with

No associations

Rating

The brightness temperatures of solar type III 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 The brightness temperatures of solar type III bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The brightness temperatures of solar type III bursts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1827146