Critical Fluctuations in Beam-Plasma Systems and Solar Type III Radio Bursts

被引:0
作者
Thejappa, G. [1 ]
MacDowall, R. J. [2 ]
机构
[1] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源
16TH ANNUAL INTERNATIONAL ASTROPHYSICS CONFERENCE: TURBULENCE, STRUCTURES, AND PARTICLE ACCELERATION THROUGHOUT THE HELIOSPHERE AND BEYOND | 2017年 / 900卷
关键词
ELECTRON-BEAM; RADIATION; TURBULENCE; EMISSION; WAVES;
D O I
10.1088/1742-6596/900/1/012019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is shown that the Langmuir waves are excited similar to critical fluctuations during phase transitions when the negative absorption due to electron beam traveling radially outward in the solar atmosphere is balanced by the positive absorption due to collisions in the corona and due to scattering on electron density inhomogeneities in the interplanetary medium. The effective temperature of the Langmuir fluctuations range from 10(11) to 10(13) K, explaining the majority of the type III bursts. The Rayleigh scattering and direct coupling due to density gradient as well as due to density inhomogeneities are discussed in the context of fundamental radiation and the combination scattering for second harmonic. The number density of electrons in type III beams is estimated and compared with observations. It is also shown that the stabilization of type III beams is achieved automatically since the instability does not develop in the case of critical fluctuations.
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页数:7
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