Solar wind rotation rate and shear at coronal hole boundaries: Possible consequences for magnetic field inversions

被引：0
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作者：
Pinto, R.F. [1 ,2 ]
Poirier, N. [2 ]
Rouillard, A.P. [2 ]
Kouloumvakos, A. [2 ]
Griton, L. [2 ]
Fargette, N. [2 ]
Kieokaew, R. [2 ]
Lavraud, B. [2 ,3 ]
Brun, A.S. [1 ]
机构：
[1] Département d'Astrophysique/aim, CEA/IRFU, CNRS/INSU, Univ. Paris-Saclay and Univ. de Paris, Gif-sur-Yvette,91191, France
[2] IRAP, Université de Toulouse,UPS-OMP, CNRS, 9 Av. colonel Roche, Toulouse cedex 4,31028, France
[3] Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, Allée Geoffroy Saint-Hilaire, Pessac,33615, France
来源：
Astronomy and Astrophysics | 2021年 / 653卷
关键词：
All Open Access; Hybrid Gold;
D O I：
暂无
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学科分类号：
摘要：
Solar wind
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