Current position: Home >> Scientific Research >> Paper Publications

FORMATION OF PLASMOIDS IN MULTIPLE CURRENT SYSTEMS

Release Time:2019-03-13  Hits:

Indexed by: Journal Article

Date of Publication: 2016-04-20

Journal: ASTROPHYSICAL JOURNAL

Included Journals: Scopus、SCIE

Volume: 821

Issue: 2

ISSN: 0004-637X

Key Words: instabilities; magnetic reconnection; magnetohydrodynamics (MHD); Sun: corona

Abstract: We show that in systems with multiple current sheets, the reconnection rate can increase with increasing S. This is essentially different from the result in single current sheet systems where the reconnection rate usually decreases with increasing S or is independent of S. Such a resistive fast reconnection can be applied to account for the rapid events in multiple current systems of astrophysical, solar, and magnetic fusion plasmas.

Prev One:Ion internal transport barrier in neutral beam heated plasmas on HL-2A

Next One:APTWG: The 5th Asia-Pacific Transport Working Group Meeting