Zobrazeno 1 - 10
of 17
pro vyhledávání: '"L. I. Starkova"'
Autor:
V. L. Merzlyakov, L. I. Starkova
Publikováno v:
Geomagnetism and Aeronomy. 62:859-861
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e14b7a6790f689c5f97614b9cd303d37
https://doi.org/10.1134/s0016793222070167
https://doi.org/10.1134/s0016793222070167
Autor:
V. L. Merzlyakov, L. I. Starkova
Publikováno v:
Geomagnetism and Aeronomy. 61:1178-1182
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0f3b1f3d74f38f24bc3838627e4bccc
https://doi.org/10.1134/s0016793221080156
https://doi.org/10.1134/s0016793221080156
Autor:
L. I. Starkova, V. L. Merzlyakov
Publikováno v:
Geomagnetism and Aeronomy. 60:831-834
The situation with the reliability of calculations of the magnetic field of the solar corona remains a topic of discussion. There is, in particular, the problem of significantly lower calculated values of the magnetic field than those recorded near t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::48e451bb3f840e38e6468b47139efbc8
https://doi.org/10.1134/s0016793220070178
https://doi.org/10.1134/s0016793220070178
Autor:
L. I. Starkova, V. L. Merzlyakov
Publikováno v:
Geomagnetism and Aeronomy. 59:1103-1107
The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the geometry of the helmet axis was used as an indicator of the configuration change. The p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7f28ebef241e9263347a1fdcdb05a5f5
https://doi.org/10.1134/s0016793219080127
https://doi.org/10.1134/s0016793219080127
Publikováno v:
Serbian Astronomical Journal, Vol 2019, Iss 199, Pp 83-87 (2019)
Ground-based total solar eclipse observations are still the key method for coronal investigations. The question about its white-light degree of polarization remains unanswered. There are hypotheses claiming that the degree of polarization in certain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::213d70381ee130584d71a1984a4bee46
https://doi.org/10.2298/saj190620005m
https://doi.org/10.2298/saj190620005m
Autor:
L. I. Starkova, V. L. Merzlyakov
Publikováno v:
Geomagnetism and Aeronomy. 56:1036-1039
The magnetic flux longitudinal distribution in the equatorial solar zone has been studied. The magnetic synoptic maps of the Wilcox Solar Observatory (WSO) during Carrington rotations (CRs) 2052–2068 in 2007 and early 2008 have been analyzed. The l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::806f45490ac41faeb9df72264faaf75a
https://doi.org/10.1134/s0016793216080156
https://doi.org/10.1134/s0016793216080156
Autor:
V. L. Merzlyakov, L. I. Starkova
Publikováno v:
Geomagnetism and Aeronomy. 55:1066-1070
The features of the longitudinal inhomogeneity of the solar magnetic field strength in the region of its generation at mid-latitudes are investigated. For this purpose, the configuration of the large-scale magnetic field was analyzed, which is determ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5573b5ddc01fa9be2d938d799a06320a
https://doi.org/10.1134/s0016793215080198
https://doi.org/10.1134/s0016793215080198
Autor:
V. L. Merzlyakov, L. I. Starkova
Publikováno v:
Geomagnetism and Aeronomy. 53:1035-1038
The interrelation between the density inhomogeneity and the magnetic field configuration in the solar corona has been studied. The situation of consistency with the regular cellular magnetic field organization, established by the authors based on pol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::77aa865b4300247c99ea3c8ab5916ad1
https://doi.org/10.1134/s001679321308015x
https://doi.org/10.1134/s001679321308015x
Autor:
V. L. Merzlyakov, L. I. Starkova
Publikováno v:
Geomagnetism and Aeronomy. 52:908-912
The configuration of the solar corona magnetic field has been studied. Data on the position of the K-corona emission polarization plane during the solar eclipses of September 21, 1941; February 25, 1952; and August 1, 2008, were used as an indicator
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5acd5811f6fa30a8c52094caece548f3
https://doi.org/10.1134/s0016793212070134
https://doi.org/10.1134/s0016793212070134
Publikováno v:
Astronomy Reports. 53:275-280
The effect of the auroral ring on the polarization of the solar corona during the solar eclipse of March 29, 2006 is studied. The angle and degree of polarization for emission arising from the combination of two partially polarized components is calc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bfb4df198c465d36112cf281903231b5
https://doi.org/10.1134/s1063772909030093
https://doi.org/10.1134/s1063772909030093