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Spectroscopic diagnostics for solar ionsWe present new calculations for several solar ions in the temperature range 10(exp 5) is less than T is less than 10(exp 6) K and discuss their diagnostic applications with the help of available observational data. In particular, we rediscuss the plasma density and temperature in the source region of the solar wind. We also study the variation of relative elemental abundances in the solar atmosphere and compare them with previous studies.
Document ID
19960021385
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Dwivedi, B. N.
(Banaras Hindu Univ. Varanasi, India)
Mohan, Anita
(Banaras Hindu Univ. Varanasi, India)
Date Acquired
August 17, 2013
Publication Date
June 30, 1995
Publication Information
Publication: International Solar Wind 8 Conference
Subject Category
Solar Physics
Accession Number
96N24781
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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