Quasi-parallel Shock Structure and Processes

By D. Burgess, E. Lucek, M. Scholer, S. Bale, M. Balikhin, A. Balogh, T. Horbury, V. Krasnoselskikh, H. Kucharek, B. Lembége and 4 more. 2005

150 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/e54c465298bd31e14055b2b15cdba2b12f83bd08

How researchers see this paper

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In Astronomy and Astrophysics

1. Mats André
2. E. Kilpua
3. A. Balogh
4. Andris Vaivads
5. Ying Liu
6. Florian Mozer
7. R. Steiger
8. A. Retinò

Citations in the corpus

• In situ evidence of magnetic reconnection in turbulent plasma (2007, background): “The turbulence is stronger when the magnetic field in the solar wind is directed approximately along the shock normal, the so-called quasi-parallel shoc”
• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “Quasi-parallel shocks feature an extended foreshock and wave activity, and as a consequence, the shock transition is more gradual than at quasi-perpendicular shocks (e.g., Bale et al. 2005; Burgess et al. 2005; Lucek et al. 2008; Kilpua et al. 2015a).”