Zobrazeno 1 - 10
of 14
pro vyhledávání: '"V. M. Malashchuk"'
Publikováno v:
Geomagnetism and Aeronomy. 61:S1-S8
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::502b3a8907bc8b2fdd6776790885500a
https://doi.org/10.1134/s001679322133001x
https://doi.org/10.1134/s001679322133001x
Publikováno v:
Geomagnetism and Aeronomy. 61:S62-S66
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b9b6a12c796b6b047e79588355bf262e
https://doi.org/10.1134/s0016793221330021
https://doi.org/10.1134/s0016793221330021
Publikováno v:
Geomagnetism and Aeronomy. 60:1067-1070
The possibility that large-scale coronal loops of solar-type stars and M dwarfs make a significant contribution to the white-light continuum emission is considered. It is shown that that the existence of high-density (>1012 cm–3) coronal loops cont
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f8f8e6082b45ec4b0f14327191927d90
https://doi.org/10.1134/s0016793220080253
https://doi.org/10.1134/s0016793220080253
Autor:
O. A. Andreeva, V. M. Malashchuk
Publikováno v:
Geomagnetism and Aeronomy. 60:1093-1100
The dynamics of coronal holes (CHs) during the declining phase of solar cycle 24 is studied based on observational data from the Atmospheric Imaging Assembly (AIA), the 19.3 nm channel, of the Solar Dynamic Observatory (SDO). Some features of changes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::107581eaa3c526de5768f690ef0f031e
https://doi.org/10.1134/s0016793220080022
https://doi.org/10.1134/s0016793220080022
Publikováno v:
Geomagnetism and Aeronomy. 58:916-924
Analysis of images of the full solar disk obtained by ground-based (BST-2, CrAO RAS) and space-based (SDO/AIA, SDO/HMI) instruments and the potential approximation method revealed some features of the evolution of a long-lived coronal hole (CH) of 20
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a02fdd96809854abe180e77ddee000be
https://doi.org/10.1134/s0016793218070022
https://doi.org/10.1134/s0016793218070022
Publikováno v:
Proceedings of the 23rd All-Russia Conference on Solar and Solar-Terrestrial Physics.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5c1d51faa7905d6452160802839e4171
https://doi.org/10.31725/0552-5829-2019-431-434
https://doi.org/10.31725/0552-5829-2019-431-434
Publikováno v:
Bulletin of the Crimean Astrophysical Observatory. 110:149-160
Questions of the mounting and adjustment of a tower solar telescope are considered through the example of the TST-2 telescope of the Crimean Astrophysical Observatory Scientific Research Institute. The authors describe the optical circuits of the tel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d855ccb18391717889749d910895dc05
https://doi.org/10.3103/s0190271714010227
https://doi.org/10.3103/s0190271714010227
Autor:
N. N. Stepanian, V. M. Malashchuk
Publikováno v:
Bulletin of the Crimean Astrophysical Observatory. 109:98-103
Magneto-isolated complexes were found in the upper chromosphere from observations in the He I λ 1083 nm line. All the complexes were confidently identified in the corona from the images in the FeIX-X λ 17.1 nm line. The boundaries of the complexes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a34b3c0207dcea743c30c5b52a999ee
https://doi.org/10.3103/s0190271713010142
https://doi.org/10.3103/s0190271713010142
Publikováno v:
Bulletin of the Crimean Astrophysical Observatory. 109:104-110
The magnetic connections of solar formations inside magneto-isolated complexes with areas outside the complexes were determined from the loop structures in the upper chromosphere and corona, as well as from calculations of magnetic field lines. It wa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::21e79dd2098416afa9d906382447f6dd
https://doi.org/10.3103/s0190271713010063
https://doi.org/10.3103/s0190271713010063
Publikováno v:
Bulletin of the Crimean Astrophysical Observatory. 108:70-77
We propose the concept of a large-scale complex of solar formations with an isolated magnetic field. The complex involves a group of coronal holes, active regions, and regions with intermediate characteristics between a coronal hole and the undisturb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::60a24148017ef25cf32e6868b701babd
https://doi.org/10.3103/s0190271712010184
https://doi.org/10.3103/s0190271712010184