Auroral Plasma Physics
By G. Paschmann, S. Haaland, Rudolf A. Treumann. 2002
278 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/88737b721bbd0d14fe18ca8f4c21448e7837b1ff
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In Astronomy and Astrophysics
- V. Sergeev
- R. McPherron
- R. Nakamura
- J. Mcfadden
- Tuija I. Pulkkinen
- Wolfgang Baumjohann
- Juhani Birn
- V. Angelopoulos
In Molecular Biology
- V. Sergeev
- Tuija I. Pulkkinen
- Juhani Birn
- R. Nakamura
- R. McPherron
- J. Arons
- Wolfgang Baumjohann
- V. Angelopoulos
Citations in the corpus
- Substorm Current Wedge Revisited (2015, background): “Omega bands have been found to grow simultaneously over a longitudinal range of several magnetic local time (MLT) hours, covering a wide range of the central to eastern portion of the SCW (e.g., Paschmann et al. 2003, Sect.”
- Particle Acceleration in the Magnetotail and Aurora (2012, background): “A general expression of the parallel electric field from the equations (15)– (20) is given by Thompson and Lysak (1996), Stasiewicz et al. (2000), and Paschmann et al. (2003): E‖ = ( R2c − λ2e 1 + k2⊥R2c 1 + k2⊥λ2e ) ∂ ∂s (∇⊥ · E⊥) (21) where s is the coordinate in the direction of the magnetic…”
- How important are dispersive Alfvén waves for auroral particle acceleration? (2007, background): “The means by which electrons are accelerated into the ionosphere with sufficient energy and flux to stimulate such features is an area of ongoing research [Paschmann et al., 2003].”
- The Jovian Auroral Distributions Experiment (JADE) on the Juno Mission to Jupiter (2017, unknown): “…terrestrial magnetospheric observations over the poles at Earth (e.g. from the FAST spacecraft, see reviews by Carlson et al. 1998; and chapters in Paschmann et al. 2003) and from previous observations in Jupiter’s equatorial region (reviewed by Khurana et al. 2004; Krupp et al. 2004) as well as…”
- Pulsar Wind Nebulae as Cosmic Pevatrons: A Current Sheet’s Tale (2012, background): “5 For a review of such phenomena, see Paschmann et al. (2002). Of particular significance to pulsars is the fact that the field aligned currents that power narrow auroral arcs consist of precipitating electron beams launched from the reconnection region in the distant magnetotail and counterstreamin”