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Proceedings Paper

High-n solar recombination lines
Author(s): Bruna I. Grimberg
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Paper Abstract

We plan to observe solar recombination lines of hydrogen H39a (2.70mm), H40a (2.92mm), H41a 3.15mm), H42a (3.38mm) at FCRAO for oaring distance from disk center to limb. Preliminar calculations following the Hoang-Binh model (1982) show a turn from emission lines into absorption lines around n=38.

Paper Details

Date Published: 30 November 2017
PDF: 2 pages
Proc. SPIE 2250, International Conference on Millimeter and Submillimeter Waves and Applications 1994, 22508O (30 November 2017); doi: 10.1117/12.2303329
Show Author Affiliations
Bruna I. Grimberg, Univ. of Massachusetts at Amherst (United States)


Published in SPIE Proceedings Vol. 2250:
International Conference on Millimeter and Submillimeter Waves and Applications 1994
Mohammed N. Afsar, Editor(s)

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