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2005), spatial relationship between twist in active region magnetic fields and solar flares, astrophysTwisted magnetic field lines in solar active regions constitute stressed flux systems, the reconnection of which can release the stored (excess) magnetic energy in the form of...
général - core.ac.uk - PDF: citeseerx.ist.psu.edu
High-resolution millimeter-wave mapping of linearly polarized dust emission: magnetic field structure... This abrupt change in polarization direction is not necessarily the signpost of a twisted magnetic field....
... former group members:... c) Magnetic field lines, showing a highly tangled and twisted magnetic field structure typical of the small-scale dynamo; yellow: 0.5mG,...
# 2005. the american astronomical society. all rights reserved. printed in u.s.a. spatial relationship between twist in active region magnetic fields and solar flaresTwisted magnetic field lines in solar active regions constitute stressed flux systems, the reconnection of which can release the stored (excess) magnetic energy in the form of...
Large polar caps for twisted magnetosphere of rotating magnetars... For a twisted magnetic field, the field lineswill inflate in the radial direction....
 PDF: arxiv.org

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sciences naturelles et appliquées / électronique et électrotechnique / informatique et traitement des données / transport terrestre - iate.europa.eu
électronique et électrotechnique - iate.europa.eu
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général - iate.europa.eu
général - iate.europa.eu
général - iate.europa.eu


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