Author： Jiling H.
Publisher： Springer Publishing Company
ISSN： 0038-0938
Source： Solar Physics, Vol.178, Iss.1, 1998-02, pp. : 179-182
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
When ion-acoustic turbulence is fully developed, Coulomb collision damping and Landau collisionless damping can all be neglected. Since the electric field force is greater than the damping force, a coronal transient can be created by the acceleration caused by the electric field. Eruptive prominence and coronal mass ejection (CME) events can occur as a consequence of this mechanism.
Related content
Coronal Transients in Radio and X-rays
By Kundu M.R.
Astrophysics and Space Science, Vol. 243, Iss. 1, 1996-01 ,pp. :
Access to resources
Recommend
Study of Coronal Transients in Uv Line Emission
By Martin R. Maccari L. Noci G.
Solar Physics, Vol. 172, Iss. 1-2, 1997-05 ,pp. :
Radio and X-ray Imaging Observations of Solar Flares and Coronal Transients
By Kundu M.R.
Solar Physics, Vol. 169, Iss. 2, 1996-12 ,pp. :
The Relationship of Green-Line Transients to White-Light Coronal Mass Ejections
By Plunkett S. Brueckner G. Dere K. Howard R. Koomen M. Korendyke C. Michels D. Moses J. Moulton N. Paswaters S. St. Cyr O. Socker D. Wang D. Simnett G. Bedford D. Biesecker D. Eyles C. Tappin S. Schwenn R. Lamy P. Llebaria A.
Solar Physics, Vol. 175, Iss. 2, 1997-10 ,pp. :