Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Yu. T. Tsap"'
Autor:
E. A. Isaeva, Yu. T. Tsap
Publikováno v:
Odessa Astronomical Publications, Vol 30, Iss 0, Pp 222-225 (2017)
Coronal mass ejections (CMEs) mostly affect the geomagnetic field. These structures are observed and studied with coronagraphic images thereforewe don’t see the corona in the plane of the sky and the measurements of the propagation speed for solar
Externí odkaz:
https://doaj.org/article/f854bf10e74f4dcaa7c29f63243641aa
Publikováno v:
Geomagnetism and Aeronomy. 62:992-996
Publikováno v:
Geomagnetism and Aeronomy. 62:997-1000
Publikováno v:
Geomagnetism and Aeronomy. 61:1045-1051
Publikováno v:
Geomagnetism and Aeronomy. 61:1052-1056
Publikováno v:
Geomagnetism and Aeronomy. 61:S62-S66
Publikováno v:
Geomagnetism and Aeronomy. 61:993-1000
Publikováno v:
Geomagnetism and Aeronomy. 61:1035-1037
Autor:
Yu. T. Tsap, Z. S. Akhtemov
Publikováno v:
Astronomy Letters. 47:117-122
Based on the data obtained with the CHIMERA algorithm, we consider the evolution of a long-lived low-latitude coronal hole during its central meridian passage over the period from February 15, 2012, to October 14, 2012. The correlation coefficient be
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