NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Computed profiles of the solar C I multiplets at 1561 and 1657 AA nine-level atomic model is presented for C I lines synthesis in the sun. All the atomic parameters are based on recent experimental and theoretical data. Profiles of the multiplets at 1561 and 1657 A are computed from a model of the solar chromosphere. The sensitivity of the results to changes in the atomic parameters is examined. Partial frequency redistribution must be included in these lines to obtain agreement between calculated and observed profiles.
Document ID
19900025116
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/167979
Authors
Mauas, Pablo J. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Avrett, Eugene H. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Loeser, Rudolf (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 14, 2013
Publication Date
October 15, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 345
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
90A12171
Funding Number(s)
CONTRACT_GRANT: NSG-7054
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available