Zobrazeno 1 - 6
of 6
pro vyhledávání: '"N. I. Shtertser"'
Publikováno v:
Astrophysics. 63:421-429
The physical conditions in the chromosphere of polar and equatorial coronal holes in the decay phase of the 24-th solar activity cycle are studied. Models of the chromosphere are constructed based on the intensities of the HeI 10830 A and Hα lines a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::255d19f82de6da3eb0cb6e038735b601
https://doi.org/10.1007/s10511-020-09646-z
https://doi.org/10.1007/s10511-020-09646-z
Publikováno v:
Astrophysics. 62:226-233
Observations in the HeI 10830 A and Hα lines are used to study the physical conditions in a polar coronal hole. The coronal hole was observed in the northern hemisphere from June 2015 through March 2017. The range of intensity variations in the coro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9a3fef35c954d6c6d24f9030b6853fc5
https://doi.org/10.1007/s10511-019-09576-5
https://doi.org/10.1007/s10511-019-09576-5
Publikováno v:
Proceedings of the 24th All-Russia Conference on Solar and Solar-Terrestrial Physics.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9bab9ef3d09b8b6ba8fe25e6e2e5f08a
https://doi.org/10.31725/0552-5829-2020-69-72
https://doi.org/10.31725/0552-5829-2020-69-72
Publikováno v:
Astronomy Reports. 61:74-79
Bright bands are observed along filaments in the He I 1083 nm line, while both bright and dark bands are observed along Hα 656.3 nm filaments. The range of brightness variations near He I filaments is 1.005–1.10 times the unperturbed brightness, w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f340ea56af59e8aff8ea893ce8ddef50
https://doi.org/10.1134/s1063772916120039
https://doi.org/10.1134/s1063772916120039
Publikováno v:
Bulletin of the Crimean Astrophysical Observatory. 104:67-78
Based on the developed method of jointly using data on the magnetic fields and brightness of fila- ments and coronal holes (CHs) at various heights in the solar atmosphere as well as on the velocities in the photosphere, we have obtained the followin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2d9014718c074f0746727edbf119cd21
https://doi.org/10.3103/s0190271708010105
https://doi.org/10.3103/s0190271708010105
Autor:
V. G. Fainshtein, V. M. Malashchuk, R. K. Zhigalkin, N. N. Stepanian, Sergey Kuzin, N. I. Shtertser, G. V. Rudenko, A. A. Pertsov, V. A. Perebeinos, I. A. Zhitnik
Publikováno v:
Solar System Research. 42:83-89
The relationship between two classes of coronal holes and high-speed quasi-stationary streams of solar wind at the Earth’s orbit is investigated. “Open” coronal holes, whose area is invariable or increases with the height over the solar surface
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c4b4bf16395eac5affb90d72f99683d1
https://doi.org/10.1134/s0038094608010097
https://doi.org/10.1134/s0038094608010097