On the solar magnetic field polarity reversal during the activity cycle

Autor:	K. I. Nikolskaya, E. I. Mogilevsky
Rok vydání:	2004
Předmět:	Polarity reversal Physics Space and Planetary Science Extreme ultraviolet Phase (waves) Activity cycle Coronal hole Astronomy and Astrophysics Astrophysics Interplanetary magnetic field Corona Magnetic field
Zdroj:	Proceedings of the International Astronomical Union. 2004:129-130
ISSN:	1743-9221 1743-9213
DOI:	10.1017/s1743921304005381
Popis:	Solar magnetic field polarity reversal (SMFPR) happens every 10-11 years. However untill now there is no clear understanding in what way this process is carried out. Results represented here are a by-product of the coronal hole study based on taken from Web-archive XUV corona images (Yohkoh and EIT/SOHO), white-light corona pictures(SOHO/LASCO) and Kitt Peak coronal hole (CH) 1083 nm maps. Observations used cover the minimum, maximum and a part of declining phase of 23-d cycle (1996-2004).To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::30ab30873817d5fa81f33d5126b2e480 https://doi.org/10.1017/s1743921304005381 Zobrazit plný text záznamu Plný text ve formátu PDF