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Numbers of Electrons in Solar Flares as Deduced from Microwave and X-Ray Bursts

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摘要 We discuss Whether the numbers of x-ray and radio-produced electrons in solar flares are the same.The number of the radio-produced electrons that is estimated with an inhomogeneous source increases by a factor of 10^(3)-10^(4) because of the inhomogeneity and the decreased magnetic field(B=120 G)of the radio source.The number of the x-ray-produced electrons decreases by a factor of 10-30 due to the increase of the number density of ions(3 × 10^(10)cm^(-3)).These are the reasons why the number of radio-produced electrons is approximately equal to that of x-ray produced in the 1981 April 27 burst.
作者 YU Xing-Feng YAO Jin-Xing 于兴凤;姚金兴(Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008;tional Astronomical Observatory,Chinese Academy of Sciences)
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2001年第3期455-457,共3页 中国物理快报(英文版)
基金 Supported by the National Natural Science Foundation of China under Grant No.19833050 the Jiangsu Natural Science Foundation(BK97207) the 95 Major Project of Chinese Academy of Sciences.
关键词 SOURCE SOLAR SOURCE
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