On some methods of estimation of solar structure rotation from observations of the Sun in the line HE λ X 1083 nm
|1Zyelyk, Ya.I, 2Stepanian, NN, 2Andryeyeva, OA |
1Space Research Institute of the National Academy of Sciences of Ukraine and the State Space Agency of Ukraine, Kyiv, Ukraine
2Scientific-Research Institute “Crimean Astrophysical Observatory” of the Ministry for Education and Science of Ukraine, Nauchny, AR Crimea, Ukraine
|Kosm. nauka tehnol. 2006, 12 ;(1):085-089|
|Publication Language: Russian|
We obtained latitudinal distributions of the rotation periods in the interval from 20 to 35 days and the capacity absorbed during these periods in the certain latitudinal zones for three types of the solar structures observable in the line He I of X 1083 nm in the top chromosphere during the time interval greater than 26 years.
|Keywords: capacity, latitudinal zones, rotation periods|
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