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Profile of the 9.85-GHz Neutral Hydrogen Line Taking into Account the Zeeman Effect (Computations and Solar Observations)
Authors:Dravskikh  A. F.  Peterova  N. G.  Topchilo  N. A.
Affiliation:1.Special Astrophysical Observatory of Russian Academy of Sciences, St. Petersburg, Russia
;2.Department of Astrophysics, St. Petersburg State University, St. Petersburg, Russia
;
Abstract:Astronomy Reports - The 9.85-GHz (3.04 cm) line of atomic hydrogen due to the 22P3/2–22S1/2 transition between levels of the hyperfine structure occupies a special place in the complex...
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