NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Heating-related flows in cool solar loopsThe effects of spatial and temporal variations in the heating of cool loop models are investigated in an attempt to explain the net redshifts that are observed on the sun. The response of initially static cool loops to changes in the energy input is simulated. For hot loops, it is found that spatially asymmetric changes produce a final steady state that is dynamic, and that spatially symmetric changes produce a final state that is static. Some general properties of cool loop equilibria are discussed, emphasizing the relationship between structure and energy input. The results are unable to explain the net redshifts observed in emission lines formed near 100,000 K on the sun.
Document ID
19880046309
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Klimchuk, J. A.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Mariska, J. T.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Date Acquired
August 13, 2013
Publication Date
May 1, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 328
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
88A33536
Funding Number(s)
CONTRACT_GRANT: NAS8-37334
CONTRACT_GRANT: N00014-85-K-0111
CONTRACT_GRANT: NGL-05-020-272
Distribution Limits
Public
Copyright
Other

Available Downloads

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