摘要
用非均匀模型，对１９８１年４月２７日０８００１Ｔ大耀斑进行了分析。从硬Ｘ射线和微波爆发的观测频谱出发，在假定周围离子密度ｎｉ＝３×１０１０／ｃｍ３的情况下，计算得到两者的总电子数ＮＸ和ＮＲ是近似相等的。这表明，至少对这个耀斑，两者的非热电子可能有同样的分布。此外，文中也分析了ＮＲ提高了１０３－１０４倍的原因可能在于磁场的非均匀性和源中的磁场值较小。
The question of whether the numbers of X-ray and radio-producing electrons in solar flares are the same has been discussed in this paper. Calculation shows that the number of radio-producing electrons NR estimated with nonhomogeneous radio source is approximately equal to the number of X-ray-producing electrons NX for the 1981 April 27 flare. It seems that they have a common population. In addition, the causes of NR increased by a factor of 103 - 104 have been analysed.
基金
国家自然科学重点基金
江苏省基金
