Evidence for the regulation of solar wind heat flux at 1 AU

Evidence for the regulation of solar wind heat flux at 1 AU
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1 AU 太阳风热通量调节的证据

DOI:
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发表时间:
1976
期刊:
影响因子:
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通讯作者:
S. M. Zink
S. M. Zink
中科院分区:
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文献类型:
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作者:
W. Feldman;J. Asbridge;S. Bame;S. Gary;M. D. Montgomery;S. M. Zink

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在1 Au处,对Imp 6合并的等离子体和磁场数据的前4个月进行了搜索,以寻找太阳风热通量(Q)局部调节的证据。从几个延长时间段的数据以及统计分析表明,阿尔芬速度有时是Q的主要调节因子,其关系为Q ΔVc = αVA。其中ΔVc是低能电子峰值与体等离子体速度之间的速度差,VA是局部阿尔芬速度,α是1阶无量纲参数。
The first 4 months of Imp 6 merged plasma and magnetic field data have been searched for evidence of local regulation of the solar wind heat flux (Q) at 1 AU. Data from several extended time periods as well as a statistical analysis suggest that the Alfven speed is at times a prime regulating factor of Q through the relation Q ∝ ΔVc = αVA. Here ΔVc is the velocity difference between the peak of the low-energy electrons and the bulk plasma velocity, VA is the local Alfven speed, and α is a dimensionless parameter of order 1.