Identifying the plasmapause in IMAGE EUV data using IMAGE RPI in situ steep density gradients
By J. Goldstein, M. Spasojević, P. Reiff, B. Sandel, W. T. Forrester, Dennis L. Gallagher, Bodo W. Reinisch. 2003
146 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/66afac6be16b94bfc1ae759eb91fde6de9025d83
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In Astronomy and Astrophysics
- J. Goldstein
- B. Sandel
- D. Carpenter
- M. Spasojević
- P. Reiff
- Mark B. Moldwin
- Bodo W. Reinisch
- Dennis L. Gallagher
In Atmospheric Science
Citations in the corpus
- Space Weather: Terrestrial Perspective (2007, background): “In the vicinity of this boundary, the plasma density has a sharp gradient; this is known as the plasmapause (Goldstein et al., 2003).”
- Global response of the plasmasphere to a geomagnetic disturbance (2003, background): “The additional time delay for the IMF Bz is attributed to a combination of the delay due to propagation from the magnetopause to the ionosphere and the ionospheric reconfiguration time [Goldstein et al., 2003b, and references therein].”
- Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere (2003, methodology): “Such an investigation has been undertaken by Goldstein et al. (2002c), who studied an erosion event on 10 July 2000, between 04:24 and 09:32 UT.”
- Simultaneous remote sensing and in situ observations of plasmaspheric drainage plumes (2004, methodology): “The average EUV lower threshold is known (in terms of total electron density) to be 40 e cm 3 [Goldstein et al., 2003c].”
- Control of plasmaspheric dynamics by both convection and sub‐auroral polarization stream (2003, methodology): “In each panel is an EUV image that has been mapped to the magnetic equator [Goldstein et al., 2003b].”
- Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, background): “Driven by an enhanced solar wind electric field, the onset of erosion requires 10–30 minutes to propagate from the magnetopause to the inner magnetosphere through the ionosphere (Goldstein et al. 2003a; Murakami et al. 2007).”