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题名: MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION
作者: ZHANG, ZD ; LI, XQ ; SMARTT, RN
刊名: ASTROPHYSICS AND SPACE SCIENCE
出版日期: 1995
卷号: 226, 期号:1, 页码:31—46
学科分类: 天文和天体物理
英文摘要: The subtle interactions between the magnetohydrodynamics (MHD) and transverse plasmons are investigated. It is shown that there is a resistive instability by the plasmon's soliton in a current sheet, which eventually turns into an eruptive instability at the magnetic field reconnection. In the case of ion-acoustic turbulence, the high temperature current sheet model must adopt the aromalous conductivity instead of the Coulomb conductivity. The numerical results are consistent with the observations obtained by Hanaoka (1994), Thus the Rare caused by X-ray loop coalescence can be basically interpreted by this model of magnetic field reconnection driven by ponderomotive force.
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/8492
Appears in Collections:期刊(老文献)_期刊论文

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ZHANG, ZD; LI, XQ; SMARTT, RN.MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION,ASTROPHYSICS AND SPACE SCIENCE,1995,226(1):31—46
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文件名: 1995029MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION.pdf
格式: Adobe PDF
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