Some features of solar spike burst generation

Details Some features of solar spike burst generation Some features of solar spike burst generation

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....39..107z&link_type=abstract

Astronomy and Astrophysics, vol. 39, no. 1, Feb. 1975, p. 107-111.

Astronomy and Astrophysics

Astrophysics

23

Harmonic Generations, Plasma Waves, Radio Bursts, Type 3 Bursts, Circular Polarization, Electron Beams, Fine Structure, Harmonic Analysis, Plasma Frequencies

Scientific paper

The generation of spike bursts is investigated. It is assumed that these bursts are caused by plasma waves excited in the process of the quasi-linear relaxation of the electron stream in the solar corona. The time evolution of bursts and their association with Type III radio emission are considered. The possibility of rather short-lived bursts corresponding to the second harmonic of the plasma frequency is pointed out. It is noted that the induced scattering of plasma waves, accompanied by a decrease in the wave number, is essential to an explanation of the strong polarization that the bursts are observed to have.

Affiliated with

Also associated with

No associations

Rating

Some features of solar spike burst generation 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 Some features of solar spike burst generation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some features of solar spike burst generation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-998143