Global response of the plasmasphere to a geomagnetic disturbance
By M. Spasojević, J. Goldstein, D. Carpenter, Umran S. Inan, B. Sandel, Mark B. Moldwin, Bodo W. Reinisch. 2003
160 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/3eaa49ffd401c9d748c99209dd61000983352af1
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In Astronomy and Astrophysics
Citations in the corpus
- Timescales for radiation belt electron acceleration and loss due to resonant wave‐particle interactions: 2. Evaluation for VLF chorus, ELF hiss, and electromagnetic ion cyclotron waves (2007, methodology): “Parenthetically, we note the recent resurgence in studies of plasmaspheric plumes [e.g., Spasojevic et al., 2003; Moldwin et al., 2004; Goldstein et al., 2004, 2005].”
- Global simulation of EMIC wave excitation during the 21 April 2001 storm from coupled RCM‐RAM‐HOTRAY modeling (2010, background): “Electron density inside such storm time plumes exhibits fine‐scale structures [Goldstein et al., 2004, Spasojević et al., 2003, 2004].”
- Simultaneous remote sensing and in situ observations of plasmaspheric drainage plumes (2004, background): “The existing EUV database contains many examples of plumes during and/or after geomagnetic disturbance times [Burch et al., 2001a, 2001b; Foster et al., 2002; Goldstein et al., 2002, 2003a, 2003c, 2003b; Sandel et al., 2004; Moldwin et al., 2004; Spasojević et al., 2003, 2004].”
- Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, background): “On smaller scale, many stormtime features have yet to be explained; for example, crenulations are a few-tenths-RE modulation of the plasmapause location that are often seen between the dawnside terminator and the westmost edge of a plume (Spasojević et al. 2003; Goldstein and Sandel 2005).”
- Space Weather: Terrestrial Perspective (2007, background): “5RE/h, with the changes following the interplanetary magnetic field variations with 20 – 30 min delay (Spasojević et al., 2003).”
- Electron scattering by whistler-mode ELF hiss in (2008, methodology): “The azimuthal spread of a particular plume varies during its evolution and is typically 0.1 RE to 1.5 RE or more [e.g., Spasojeviç et al., 2003; Darrouzet et al., 2006].”
- A statistical look at plasmaspheric drainage plumes (2008, background): “[53] The fact that plasmaspheric drainage plumes are lumpy has been noted in the literature [Spasojevic et al., 2003; Moldwin et al., 2004; Goldstein et al., 2004].”