0125154 - ASU-R 20030060 RIV NL eng C - Konferenční příspěvek (zahraniční konf.)
Ambrož, Pavel
Spatial distribution, time evolution and rotation of the large-scale total magnetic flux patterns on the Sun.
Solar variability as an input to the Earth's environment. Noordwijk: ESA Publication division, 2003 - (Wilson, A.), s. 59-62. ESA Special publication., 535.
[International solar cycle studies symposium 2003. Tatranská Lomnica (SK), 23.06.2003-28.06.2003]
Grant CEP: GA ČR GA205/01/0657; GA AV ČR IBS1003006
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: solar corona * rotation * magnetic field
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

The study brings a new light on the problem of the coronal rotation. Close relationship between enhanced magnetic flux regions and the green corona bright regions is found. Generally is accepted conclusion that the corona rotate more rigidly than the solar photosphere with measurable background magnetic field. Aim of the present study is to explain possible cause of such findings.
Trvalý link: http://hdl.handle.net/11104/0023412