How do fits of simulated magnetic clouds correspond to their real shapes in 3D?

0348472 - ASÚ 2011 RIV DE eng J - Článek v odborném periodiku
Vandas, Marek - Romashets, E. P. - Geranios, A.
How do fits of simulated magnetic clouds correspond to their real shapes in 3D?
Annales Geophysicae. Roč. 28, č. 8 (2010), s. 1581-1588. ISSN 0992-7689. E-ISSN 1432-0576.
[STEREO-3/SOHO-22 Workshop: Three Eyes on the Sun, Multi-spacecraft studies of the corona and impacts on the heliosphere. Bournemouth, 27.04.2009-01.05.2009]
Grant CEP: GA ČR GA205/09/0170; GA MŠMT ME09032
Grant ostatní: ESA(XE) ESA-PECS project No.98068
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: interplanetary magnetic fields * magnetic clouds * numerical simulations
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 1.620, rok: 2010

Trvalý link: http://hdl.handle.net/11104/0189001