PMO OpenIR  > 期刊(老文献)
日珥磁场结构的Rayleigh-Tayler不稳定性和无黑子双带耀斑
曹天君 ; 许敖敖 ; 成中杰
1982
Source Publication天文学报
ISSN0001-5245
Volume23Issue:3Pages:203-210
Abstract本文讨论了,分析彗尾亮度而求出的“修正的γ-分布函数”f(γ)的意义,f(γ)与尘埃模型的物理量的关系,以及f(γ)做为检验尘埃模型的手段的有效性。根据文[1]所提方法,详细考虑了该方法中存在的各种因数,求出高精度的“修正的γ-分布函数”f(γ)。对Arend-Roland彗星求得的f(γ)函数是γ=0.10和0.01,相对高度为1:0.6的双峰分布。假设粒子抛射率反比于彗核太阳距离的平方,一天文单位时的粒子抛射率P_d,将是P_d
Keyword不稳定性 双带耀斑 磁场结构 暗条电流 磁力线 中性电流片 活动区磁场 黑子群 磁场强度 磁场梯度
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7469
Collection期刊(老文献)
Recommended Citation
GB/T 7714
曹天君,许敖敖,成中杰. 日珥磁场结构的Rayleigh-Tayler不稳定性和无黑子双带耀斑[J]. 天文学报,1982,23(3):203-210.
APA 曹天君,许敖敖,&成中杰.(1982).日珥磁场结构的Rayleigh-Tayler不稳定性和无黑子双带耀斑.天文学报,23(3),203-210.
MLA 曹天君,et al."日珥磁场结构的Rayleigh-Tayler不稳定性和无黑子双带耀斑".天文学报 23.3(1982):203-210.
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