Altered solar wind-magnetosphere interaction at low Mach numbers: Coronal mass ejections

By B. Lavraud, J. Borovsky. 2008

159 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/25fb10b0c9b1a36df2eb5911e66232b70f1a5ae8

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In Astronomy and Astrophysics

1. M. Owens
2. E. Kilpua
3. C. Russell
4. A. Balogh
5. C. Farrugia
6. P. Démoulin
7. Jan Luhmann
8. Ying Liu

Citations in the corpus

• Multispacecraft observation of magnetic cloud erosion by magnetic reconnection during propagation (2012, background): “By contrast, since the Alfvén speed in the solar wind increases as one approaches the Sun [Fujimoto et al., 2007; Lavraud and Borovsky, 2008], and magnetic reconnection rate scales with the Alfvén speed, we may expect that a significant portion of the magnetic erosion investigated here has in fact…”
• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “also pointed out that high velocity shear at the magnetopause creates favorable conditions for non-linear Kelvin-Helmholtz vortices (Lavraud and Borovsky 2008) that may increase”