0124725 - ASU-R 20000187 RIV NL eng J - Článek v odborném periodiku
Bumba, Václav - Garcia, A. - Klvaňa, Miroslav
The role of the magnetic field in the ascension of the 22nd and 23rd cycles of activity.
Solar Physics. Roč. 197, č. 1 (2000), s. 175-202. ISSN 0038-0938. E-ISSN 1573-093X
Grant CEP: GA AV ČR IAA3003903; GA ČR GA205/97/0500; GA AV ČR KSK1003601
Výzkumný záměr: CEZ:AV0Z1003909
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 2.095, rok: 2000

We described the pattern and the forms of the minimum activity investigated, underlining the fact that the last impulses of the old activity are very short-lived, mostly of small intensity, forming a relatively large number of groups of type B and A, the magnetic orientation of which is often difficult to estimate.
Trvalý link: http://hdl.handle.net/11104/0022984