Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..174h&link_type=abstract
Acta Astrophys. Sin., Vol. 15, No. 2, p. 174 - 182
Astronomy and Astrophysics
Astrophysics
1
Plasma: Instabilities, Solar Radio Bursts: Polarization, Active Galactic Nuclei: Radio Jets
Scientific paper
On the basis of the authors' previous paper, the weakly magnetized modification for the dispersion relation of the ambient electromagnetic waves is taken into consideration. In the range of 1 < ωpe/Ωe < 10 (for the solar corona, interplanetary space and radio jets of galaxies), the growth rates of the ordinary and extraordinary modes excited directly by beam-plasma instability are calculated. The growth of the extraordinary modes is evidently restricted with the increasing ωpe/Ωe, hence, in the parameters of this paper, electromagnetic waves excited by beam-plasma instability is mainly in the ordinary modes, which can explain the polarization of type III solar bursts and the radio jets in active galactic nuclei.
Huang Guangli
Mao Ding-yi
Wang De-yu
No associations
LandOfFree
The weakly magnetized modification for the mechanism of direct amplification of electromagnetic waves by beam-plasma instability. 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 weakly magnetized modification for the mechanism of direct amplification of electromagnetic waves by beam-plasma instability., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The weakly magnetized modification for the mechanism of direct amplification of electromagnetic waves by beam-plasma instability. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1827328