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次相对论热等离子体中的回旋同步辐射 被引量:1

Cyclosynchrotron Radiation in Mildly Relativistic Hot Plasma
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摘要 利用克希霍夫定律及光深条件,考虑了等离子体的自吸收,得到了具有磁场的次相对论热等离子体的回旋同步辐射的辐射率表达式. By means of Kirchhoff's law and condition of optical depth, we found the cyclosynchrotron emission rate in mildly relativistic thermal plasma with magnetic fields.
出处 《中南民族学院学报(自然科学版)》 1997年第2期36-38,共3页 Journal of South-Central University for Nationalities(Natural Sciences)
关键词 回旋同步辐射 自吸收 次相对论 热等离子体 cyclosynchrotron radiation self absorption mildly relativistic thermal plasma ,
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  • 1周爱华.回旋同步辐射自吸收的特性[J].天文学报,2005,46(1):12-18. 被引量:1
  • 2黄光力.日冕磁场和重联的射电信号[J].天文研究与技术,2006,3(2):99-112. 被引量:1
  • 3Fleishman G D, Melnikov V F. Optically thick gyrosynchrotron emission from anisotropic electron distributions. Astrophys. J., 2003, 584(1):1071-1083
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  • 7Cairns I H, Mitchell J J, Knock S A, Robinson P A. Towards a quantitative theory for 2-3 kHz radio emission from beyond the heliopause. Adv. Space Res., 2004, 34(1):88-93
  • 8Petrosian V, Mctiernan J M. Emission, absorption and polarization of mildly relativistic particles. Phys. Fluids, 1983, 26(10):3023-3028
  • 9Petrosian V. Synchrotron emissivity from mildly relativistic particles. Astrophys. J., 1981, 251:727-738
  • 10Sakurai K. Gyrosynchrotron radiation and its transfer in a magnetoactive plasma. Astrophys. J., 1972, 174:135-149

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