Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations
By C. Cattell, J. Dombeck, J. Wygant, J. Drake, M. Swisdak, M. Goldstein, W. Keith, A. Fazakerley, Mats André, E. Lucek and 1 more. 2005
260 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/a46ef4dd3b6574f45536d92497dc89c9bb69c1de
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In Astronomy and Astrophysics
- Bengt Eliasson
- E. Zweibel
- Y. Khotyaintsev
- Alain Roux
- M. Yamada
- Andris Vaivads
- R. Ergun
- Werner Magnes
In Nuclear and High Energy Physics
Citations in the corpus
- Magnetic Reconnection in Astrophysical and (2009, background): “Lower hybrid waves were observed during reconnection in the Earth’s magnetotail (Bale, Mozer & Phan 2002; Cattell et al. 2005), as were whistler waves (Petkaki, Freeman & Walsh 2006; Wei et al. 2007).”
- The Search-Coil Magnetometer for MMS (2016, background): “…waves (electrostatic as well as electromagnetic) have been identified in the magnetotail during substorm events thanks to waveform captures at very high sampling rates onboard Cluster (e.g., Cattell et al. 2005) or THEMIS satellites (Ergun et al. 2009; Andersson et al. 2009; Tao et al. 2011).”
- The electron–cyclotron maser for astrophysical application (2006, background): “In this context it should be noted that chains of phase space holes have recently been observed (Cattell et al. 2005) in a region where magnetic reconnection was going on in the collisionless plasma sheet of the Earth’s magnetotail at roughly 15 Earth radii anti-Sunward distance behind the Earth.”
- Formation and dynamics of coherent structures involving phase-space vortices in plasmas (2006, background): “One-dimensional electron holes correlated with reconnection at the Earth’s magnetotail have been recently observed by the Cluster spacecraft [57].”
- Observation of energetic electrons within magnetic islands (2008, background): “The third criterion is based on the fact that electrons in the inflow near the X-line region are much hotter in the direction parallel to the magnetic field than in the perpendicular direction, whereas in the reconnection region such as the interior of islands the two temperatures are roughly the sa”