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Flow in coronal loops with a mass sourceThis research studies the flow of plasma inside a coronal loop in which an injection of plasma through the lateral surface is permitted. The flow is assumed steady and polytropic. The problem covers two cases: (a) upflow at one footpoint, downflow at the other; (b) downflow at both footpoints. The first case can be shown to be quite similar to that of a mass-conserving flow with variable cross section; the second, instead, is characterized by solutions with a different type of topology; its main new feature is the obvious fact that all the solutions pass through a single point going from negative to positive velocities. In this second case the density ratio between footpoints and top can be much smaller than in a mass conserving flow. This can explain some properties of observed loops.
Document ID
19840031556
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Noci, G.
(Padova, Universita Padua, Italy)
Zuccarello, F.
(Catania Osservatorio Astrofisico, Catania, Italy)
Date Acquired
August 12, 2013
Publication Date
October 1, 1983
Publication Information
Publication: Solar Physics
Volume: 88
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
84A14343
Funding Number(s)
CONTRACT_GRANT: NSF ATM-77-20580
CONTRACT_GRANT: NAS5-24420
CONTRACT_GRANT: N00014-76-C-0207
CONTRACT_GRANT: NGR-05-020-559
Distribution Limits
Public
Copyright
Other

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