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Journal of Atmospheric and Solar-Terrestrial Physics 62 (2000) 14371448 www.elsevier.nl/locate/jastp

Summary: Journal of Atmospheric and Solar-Terrestrial Physics 62 (2000) 1437≠1448
Initiation of CMEs: the role of magnetic twist
L. van Driel-Gesztelyia;b; , P.K. Manoharanc, P. D√emoulina, G. Aulanierd;e,
C.H. Mandrinif , M. Lopez-Fuentesf , B. Schmiedera;g, S. Orlandoh,
B. Thompsoni, S. Plunkettj
aObservatoire de Paris, D.A.S.O.P., F-92195, Meudon, France
bKonkoly Observatory, Budapest, Pf. 67, H-1525, Hungary
cRadio Astronomy Centre (NCRA), Tata Institute of Fundamental Research, Udhagamandalam (Ooty), India
dNRL, Code 7670, Washington, DC 20375, USA
eGMU, CSI, 4400 University Dr., Fairfax, VA 22030, USA
f IAFE-CONICET, CC.67, Suc.28, 1428 Buenos Aires, Argentina
gUniversity of Oslo, N-0315 Oslo, Norway
hOsservatorio Astronomico di Palermo "G.S. Vaiana", I-90134 Palermo, Italy
iNASA=Goddard SFC, Greenbelt, MD 20771, USA
jUSRA, Naval Research Laboratory, Washington, DC 20375, USA
Received 1 January 2000; received in revised form 28 February 2000; accepted 1 April 2000
Recent multiwavelength observations, modelling results and theoretical developments indicate the importance of twisted
magnetic conˇgurations in solar active regions (ARs) in the initiation of coronal mass ejections (CMEs). Through multiwave-


Source: Aulanier, Guillaume - Observatoire de Paris


Collections: Physics