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Simulation of magnetic cloud propagation in three dimensions
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SYSNO ASEP 0124971 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Simulation of magnetic cloud propagation in three dimensions Author(s) Vandas, Marek (ASU-R) RID, ORCID
Odstrčil, Dušan (ASU-R)
Watari, S. (JP)Source Title SOLSPA 2001. Proceedings of the second Solar Cycle and Space Weather Conference / Sawaya-Lacoste H.. - Noordwijk : ESA Publications Division, 2002 Pages s. 293-296 Number of pages 4 s. Action Solar Cycle and Space Weather Euroconference /2./ Event date 24.09.2001-29.09.2001 VEvent location Vico Equense Country IT - Italy Event type EUR Language eng - English Country NL - Netherlands Keywords magnetic clouds ; numerical simulations ; space weather Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects 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 Magnetohydrodynamic simulation is used to study evolution and propagation of loop-like magnetic clouds through interplanetary space in three dimensions. Results show that a flux rope becomes highly deformed. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2003
Number of the records: 1