In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 44, no. 2
V. Rušin - M. Saniga - R. Komžík
Detaily:
Rok, strany: 2014, 119 - 129
Kľúčové slová:
Sun, white-light corona, solar polar magnetic fields
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_44/No_2/pp119-129_abstract.html
O článku:
We discuss the large-scale structure of the solar corona, in particular its helmet streamers, as observed during total solar eclipses around maxima of solar cycles and make its comparison with solar polar magnetic field strength as observed by the Wilcox Solar Observatory (WSO) since 1976. Even though the magnetic field strength at the solar poles around cycle minima decreased minimally twice in the last forty years, distributions of helmet streamers around the Sun in different cycles around cycle maxima remain nearly the same. This indicates that large-scale magnetic structures governing the shape and evolution of helmet streamers must be of a different nature than those related with solar polar fields.
Ako citovať:
ISO 690:
Rušin, V., Saniga, M., Komžík, R. 2014. White-light corona and solar polar magnetic field strength over solar cycles. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 44, no.2, pp. 119-129. 1335-1842.
APA:
Rušin, V., Saniga, M., Komžík, R. (2014). White-light corona and solar polar magnetic field strength over solar cycles. Contributions of the Astronomical Observatory Skalnaté Pleso, 44(2), 119-129. 1335-1842.