학술논문
Compendium solar spectrum formation
Document Type
Working Paper
Author
Source
Subject
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Abstract
The solar spectrum conveys most of our diagnostics to find out how our star works. They must be understood for utilization, but solar spectrum formation is complex because the interaction of matter and radiation within the solar atmosphere suffers non-local control in space, wavelength, and time. These complexities are summarized and illustrated with classic literature. They combine in chromospheric spectrum formation.
Comment: Lingezicht Astrophysics Report 2 for a NIT Calicut solar physics school. Two-tier text split between brief main text (10 pages) and extensive yellow-page elaborations (36 pages). Version 8: 62 pages, 521 references, only few equations and figures but many more via pdf openers
Comment: Lingezicht Astrophysics Report 2 for a NIT Calicut solar physics school. Two-tier text split between brief main text (10 pages) and extensive yellow-page elaborations (36 pages). Version 8: 62 pages, 521 references, only few equations and figures but many more via pdf openers