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On non-local transport processes in the solar atmosphereWe review two mechanisms which can lend a non-local character to energy transport in the solar atmosphere, heat flux propagating in the form of collisionless electrons, and non-equilibrium ionization of hydrogen driven by ambipolar diffusion. Application of these processes to modelling of the lower transition region and upper chromosphere is considered.
Document ID
19930055896
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Macneice, P. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Electromechanical coupling of the solar atmosphere; Proceedings of the OSL Workshop, Capri, Italy, May 27-31, 1991 (A93-39876 15-92)
Publisher: American Institute of Physics
Subject Category
Solar Physics
Accession Number
93A39893
Distribution Limits
Public
Copyright
Other

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IDRelationTitle19930055879Collected WorksElectromechanical coupling of the solar atmosphere; Proceedings of the OSL Workshop, Capri, Italy, May 27-31, 1991
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