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MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION
ZHANG, ZD ; LI, XQ ; SMARTT, RN
1995
Source PublicationASTROPHYSICS AND SPACE SCIENCE
ISSN0004-640X
Volume226Issue:1Pages:31—46
AbstractThe 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.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8492
Collection期刊(老文献)
Recommended Citation
GB/T 7714
ZHANG, ZD,LI, XQ,SMARTT, RN. MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION[J]. ASTROPHYSICS AND SPACE SCIENCE,1995,226(1):31—46.
APA ZHANG, ZD,LI, XQ,&SMARTT, RN.(1995).MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION.ASTROPHYSICS AND SPACE SCIENCE,226(1),31—46.
MLA ZHANG, ZD,et al."MAGNETIC RECONNECTION MODEL FOR X-RAY FLARE LOOP INTERACTION".ASTROPHYSICS AND SPACE SCIENCE 226.1(1995):31—46.
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