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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 02/2018, Volume 610, p. A60
Journal Article
The Astrophysical journal, ISSN 0004-637X, 12/2015, Volume 814, Issue 2, pp. 99 - 9
...: the open magnetic flux. However, without running costly numerical simulations of the stellar wind, reconstructing the coronal structure of the large-scale magnetic field is not trivial... 
MHD | stars: magnetic field | stars: coronae | stars: winds, outflows | Sun: corona | stars: rotation | TOPOLOGY | FIELDS | ANGULAR-MOMENTUM EVOLUTION | INTERPLANETARY | MODEL | DRIVEN | SOURCE-SURFACE | ASTRONOMY & ASTROPHYSICS | BRAKING | STARS | DYNAMO | Stellar winds | Magnetic flux | Coronas | Stars | Mathematical models | Magnetic fields | Rotational | Stellar coronas
Journal Article
Journal Article