Chromospheric Spectroscopy
Chromospheric Spectroscopy is a specialized observational method in solar physics that analyzes spectral emissions from the Sun's chromosphere to infer its physical properties, dynamics, and thermal structure through high-resolution wavelength-resolved measurements distinct from photospheric or coronal spectroscopic techniques.
303
Publications
20K
Citations
866
Authors
324
Institutions
Publications per year
2017–2026
40
303
Chromospheric variations in main-sequence stars
S. L. Baliunas, R. A. Donahue, W. H. Soon et al. · The Astrophysical Journal · 1995 · 1K citations
Natural Sciences, Astronomy, Physics +11
Chromospheric variations in main-sequence stars
O. C. Wilson · The Astrophysical Journal · 1978 · 636 citations
Natural Sciences, Astronomy, Physics +11
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324
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
15 h-index
27 publications
1.7K citations
Osservatorio Astrofisico di Catania
Catania, Italy
14 h-index
42 publications
3K citations

Chinese Academy of Sciences
Beijing, China
14 h-index
33 publications
1.1K citations

Kitt Peak National Observatory
Tucson, United States
13 h-index
21 publications
949 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
12 h-index
53 publications
957 citations
National Astronomical Observatories
Beijing, China
11 h-index
25 publications
950 citations

Space Telescope Science Institute
Baltimore, United States
11 h-index
12 publications
1.5K citations
National Solar Observatory
Boulder, United States
11 h-index
17 publications
652 citations
1–8 of 324
ApJ · 101 publications · 7.4K citations
39
h-index
45 publications · 2.6K citations
25
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22 publications · 1K citations
18
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AJ · 22 publications · 3.4K citations
18
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24 publications · 788 citations
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