Semiempirical modeling of large-scale flow on the Sun

Number of the records: 1

SYSNO ASEP	0124814
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Ostatní články
Title	Semiempirical modeling of large-scale flow on the Sun
Author(s)	Ambrož, Pavel (ASU-R)_{RID, ORCID}
Source Title	Solar Physics. - : Springer - ISSN 0038-0938 Roč. 199, č. 2 (2001), s. 251-266
Number of pages	16 s.
Language	eng - English
Country	NL - Netherlands
Keywords	sun ; magnetic field ; horizontal flow
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA3003806 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	KSK1003601 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
CEZ	AV0Z1003909 - ASU-R
Annotation	Image of the 2-D large-scale flow on the sphere is derived from the trajectories of the independent fee testing particles driven by the derived velocity field. The horizontal flow displays a velocity gradient and an eddy structure. The sllow- and long-lived temporal evolution of the low structures is descibed.
Workplace	Astronomical Institute
Contact	Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2002

Number of the records: 1