Magnetic fields and spots of low-mass stars
A short description of a content of the solar-stellar physics is given. In this branch of astrophysics various phenomena of the solar and stellar activity as well as its evolution are considered from the united point of view. Within the framework of such an approach, the modern state of study of sur...
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| Format: | Article |
| Language: | English |
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National Aviation University
2000-10-01
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| Series: | Вісник Астрономічної школи |
| Online Access: | http://astro.nau.edu.ua/issues/2000_V.1_Iss.1/016.html |
| Summary: | A short description of a content of the solar-stellar physics is given. In this branch of astrophysics various phenomena of the solar and stellar activity as well as its evolution are considered from the united point of view. Within the framework of such an approach, the modern state of study of surface inhomogeneities on stars with an essential role of convective transfer in subphotospheric layers and results of magnetometric investigations of these stars are reviewed. |
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| ISSN: | 1607-2855 2411-6602 |