The role of magnetic reconnection in CME acceleration

Space Science Reviews

Volumn 121, Issue 1-4, 2005, Pages 33-47

  Wu, S T ^a   Zhang, T X ^a,d   Dryer, M ^b   Feng, X S ^c   Tan, Arjun ^d  

^a UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^b NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

^c CENTER FOR SPACE SCIENCE AND APPLIED RESEARCH   (China)

^d ALABAMA A AND M UNIVERSITY   (United States)

Author keywords

Acceleration; Sun: corona; Sun: coronal mass ejection (CMEs); Sun: MHd simulation

Indexed keywords

ACCELERATION; AIR EJECTORS; COMPUTER SIMULATION; KINEMATICS; MAGNETIC FIELD EFFECTS; MAGNETOHYDRODYNAMICS; TOPOLOGY;

DESTABILIZATION; SUN: CORONA; SUN: CORONAL MASS EJECTIONS (CME); SUN: MHD SIMULATION;

SPACE RESEARCH;

EID: 33744810600     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-006-6159-9     Document Type: Conference Paper

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