NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Mg I as a probe of the solar chromosphere - The atomic modelThis paper presents a complete atomic model for Mg I line synthesis, where all the atomic parameters are based on recent experimental and theoretical data. It is shown how the computed profiles at 4571 A and 5173 A are influenced by the choice of these parameters and the number of levels included in the model atom. In addition, observed profiles of the 5173 A b2 line and theoretical profiles for comparison (based on a recent atmospheric model for the average quiet sun) are presented.
Document ID
19880058912
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
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 13, 2013
Publication Date
July 15, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 330
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
88A46139
Funding Number(s)
CONTRACT_GRANT: NSG-7054
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available