Polar fields during the rising phase of cycle 22

Autor:	Haimin Wang, Frances Tang
Rok vydání:	1991
Předmět:	Physics Solar observatory Field (physics) business.industry Astronomy and Astrophysics Field strength Astrophysics Solar physics Solar cycle Magnetic field Optics Magnetogram Space and Planetary Science Astrophysics::Solar and Stellar Astrophysics Polar business
Zdroj:	Solar Physics. 132:247-256
ISSN:	1573-093X 0038-0938
DOI:	10.1007/bf00152286
Popis:	High-resolution magnetograph observations of the polar magnetic fields have been obtained at intervals of time since the end of 1986 at Big Bear Solar Observatory. The Big Bear data differ from the low-resolution, full-disk magnetograph observations in that the 2 arc sec resolution makes it possible to resolve concentrated field upward of 100 G. The purpose of this ongoing observation is to examine the evolution of polar fields during the expected polarity reversal as cycle 22 passes its maximum phase, and secondly, to study the polar magnetic field: its true field strength, distribution, and how it compares to other parts of the quiet Sun.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::b2df42dbe6ddd55a362e6415cb2ff4e3 https://doi.org/10.1007/bf00152286 Zobrazit plný text záznamu Full text from SpringerLink