Results 151 to 160 of about 302 (161)
Energy Balance in Solar and Stellar Chromospheres
The spectrum from a specific region of the sun or from a star can be used to determine the temperature-density stratification and other physical properties of the emitting atmospheric layers. We need such a description of the atmosphere in order to understand the causes of solar activity and the nature of various stellar phenomena.
Eugene H. Avrett
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Stellar and Solar Chromospheres and Attendant Phenomena
Thomas R. Ayres
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Stellar chromospheric activity in main-sequence stars
The research presented here presents a narrow slice of several largescale, ground-based astronomy surveys focused on chromospheric activity measurements of stars from the Keck Observatory. We conducted a comprehensive study analyzing chromospheric activity and its relationship with stellar properties in exoplanet host stars and solar neighborhood stars.openaire +1 more source
Stellar spectroscopy in ground-based ultraviolet. III: Chromospheres and envelopes of cool stars
Astrophysical Bulletin, 2010V E Panchuk, V G Klochkova, M V Yushkin
exaly
Stellar Model Chromospheres. H. Procyon (F5 Iv/v)
Astrophysical Journal, 1974Thomas R Ayres, Richard A Shine
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Diagnostics of stellar chromospheres and transition regions
1999Lanzafame, AC, Butler, CJ, Doyle, JG
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