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Three-dimensional MHD simulation of a loop-like magnetic cloud in the solar wind
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SYSNO ASEP 0125041 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Ostatní články Title Three-dimensional MHD simulation of a loop-like magnetic cloud in the solar wind Author(s) Vandas, Marek (ASU-R) RID, ORCID
Odstrčil, Dušan (ASU-R)
Watari, S. (JP)Source Title Journal of Geophysical Research - ISSN 0148-0227
Roč. 107, A9 (2002), s. SSH2-1 - SSH2-11Number of pages 11 s. Language eng - English Country US - United States Keywords magnetic clouds ; MHD simulations ; interplanetary magnetic fields Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects KSK3012103 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) GA205/99/1712 GA ČR - Czech Science Foundation (CSF) IAA3003003 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) IBS1003006 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z1003909 - ASU-R Annotation A magnetic cloud ejected from the Sun is simulated as a part of a toroid. Its evolution and propagation through interplanetary space are studing using three-dimensional magnetohydrodynamics self-consistent numerical simulations. The flux rope deforms as it moves from the Sun, and this deformation causes a hypothetical spacecraft to observe the flux rope two times at some location. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2003
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