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Cited article:
E. Adamson, J. Büchner, A. Otto
A&A, 557 (2013) A118
Published online: 2013-09-17
This article has been cited by the following article(s):
The 3D MHD code GOEMHD3 for astrophysical plasmas with large Reynolds numbers
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Astronomy & Astrophysics 580 A48 (2015)
DOI: 10.1051/0004-6361/201425274
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Jason E. Kooi and Molly E. Kaplan
Solar Physics 295 (8) (2020)
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The Kelvin–Helmholtz instability under Parker-Spiral Interplanetary Magnetic Field conditions at the magnetospheric flanks
E. Adamson, K. Nykyri and A. Otto
Advances in Space Research 58 (2) 218 (2016)
DOI: 10.1016/j.asr.2015.09.013
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Magnetic Connectivity in the Corona as a Source of Structure in the Solar Wind
B. L. Burkholder, A. Otto, P. A. Delamere and J. E. Borovsky
Journal of Geophysical Research: Space Physics 124 (1) 32 (2019)
DOI: 10.1029/2018JA026132
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Magnetic Reconnection of Solar Flux Tubes and Coronal Reconnection Signatures in the Solar Wind at 1 AU
B. L. Burkholder and A. Otto
Journal of Geophysical Research: Space Physics 124 (11) 8227 (2019)
DOI: 10.1029/2019JA027114
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Coronal bright points
Maria S. Madjarska
Living Reviews in Solar Physics 16 (1) (2019)
DOI: 10.1007/s41116-019-0018-8
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