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Spatial distribution, time evolution and rotation of the large-scale total magnetic flux patterns on the Sun
- 1.0125154 - ASU-R 20030060 RIV NL eng C - Conference Paper (international conference)
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]
R&D Projects: GA ČR GA205/01/0657; GA AV ČR IBS1003006
Institutional research plan: CEZ:AV0Z1003909
Keywords : solar corona * rotation * magnetic field
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
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.
Permanent Link: http://hdl.handle.net/11104/0023412
Number of the records: 1