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Mass flow velocity distribution in the solar chromosphereA study of chromospheric lines (those of Si-II and Si-III) was made using the data from high resolution telescope and spectrograph (HRTS). The optically thick line profiles such as lambda 1206 due to Si-III and lambda 1265 and lambda 1533 due to Si-II were to be investigated in detail using the techniques of spectrum synthesis in an attempt to model the mass flow velocity distribution in the region of the solar atmosphere.
Document ID
19830016182
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Tripp, D. A. (Weber State Coll. Ogden, UT, United States)
Date Acquired
September 4, 2013
Publication Date
September 30, 1981
Subject Category
Solar Physics
Report/Patent Number
NASA-CR-170744
NAS 1.26:170744
Accession Number
83N24453
Funding Number(s)
CONTRACT_GRANT: NAGW-19
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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