NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The eruption of a quiescent prominence as observed in UV linesObservations of an eruptive and a quiescent prominence are compared in order to understand better the energetic processes in an eruptive prominence. Several differences are pointed out which suggest that the activation consists not only of a mechanical movement of material, but also changes in the temperature of the prominence plasma. Some prominence material that does not seem to participate in the large-scale prominence motion is heated during the eruptive event. Most of this material is heated to transition zone temperatures with almost no cool 'core'. The behavior indicates that there are structures that are first cool and then heat up to transition zone temperatures, apparently remaining stable for some time at these temperatures.
Document ID
19900033156
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Fontenla, J. M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Poland, A. I.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Solar Physics
Volume: 123
Issue: 1 19
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
90A20211
Funding Number(s)
CONTRACT_GRANT: NAS5-28407
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available