Počet záznamů: 1
How do fits of simulated magnetic clouds correspond to their real shapes in 3D?
- 1.0348472 - 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
MHD simulations of magnetic cloud propagation are used to check our fitting procedure. Simulated spacecraft measurements are fitted by models of magnetic clouds and resulting parameters are compared with real shapes of magnetic clouds which can be directly obtained from our simulations. The comparison shows that cloud parameters are determined quite reliably for spacecraft crossings near the cloud axis.
Trvalý link: http://hdl.handle.net/11104/0189001
Počet záznamů: 1