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How deep can one see into the sun?Conventional wisdom dictates that the 1.642-micron H(-) opacity minimum is the best window to the depths of the solar photosphere. However, the violet continuum near 0.4 micron exhibits a larger intensity response to small thermal perturbations at depth, and thus might offer an even better view of the subsurface roots of granulation cells and magnetic flux tubes.
Document ID
19900033050
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ayres, Thomas R.
(Colorado, University Boulder, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Solar Physics
Volume: 124
Issue: 1 19
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
90A20105
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-07029
CONTRACT_GRANT: NGL-06-003-057
Distribution Limits
Public
Copyright
Other

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