In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 41, no. 2
M. Minarovjech - V. Rušin - M. Saniga
Detaily:
Rok, strany: 2011, 106 - 112
Kľúčové slová:
Sun: solar cycle, Sun: synoptic charts of magnetic fields
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2011/Vol_41/No_2/pp106-112_abstract.html
O článku:
Time-latitude and time-longitude distributions of solar surface magnetic fields are analyzed employing classical and modified synoptic charts. The equatorial branch in solar cycle 23 in the southern hemisphere lasted two years longer than its northern counterpart. The most remarkable finding is that in the present solar cycle a pole-ward migrating magnetic field branch is absent on the southern hemisphere, while on the northern one is well developed. This feature was not observed in previous solar cycles for the same period after cycles' onsets.
Ako citovať:
ISO 690:
Minarovjech, M., Rušin, V., Saniga, M. 2011. Synoptic charts of solar magnetic fields. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 41, no.2, pp. 106-112. 1335-1842.
APA:
Minarovjech, M., Rušin, V., Saniga, M. (2011). Synoptic charts of solar magnetic fields. Contributions of the Astronomical Observatory Skalnaté Pleso, 41(2), 106-112. 1335-1842.