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Propagation characteristics of plasma sheet oscillations during a small storm
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| Zeitschriftentitel: | Geophysical Research Letters |
|---|---|
| Personen und Körperschaften: | , , , , , , , , |
| In: | Geophysical Research Letters, 35, 2008, 17 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
American Geophysical Union (AGU)
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| Schlagwörter: |
| author_facet |
Gabrielse, C. Angelopoulos, V. Runov, A. Kepko, L. Glassmeier, K. H. Auster, H. U. McFadden, J. Carlson, C. W. Larson, D. Gabrielse, C. Angelopoulos, V. Runov, A. Kepko, L. Glassmeier, K. H. Auster, H. U. McFadden, J. Carlson, C. W. Larson, D. |
|---|---|
| author |
Gabrielse, C. Angelopoulos, V. Runov, A. Kepko, L. Glassmeier, K. H. Auster, H. U. McFadden, J. Carlson, C. W. Larson, D. |
| spellingShingle |
Gabrielse, C. Angelopoulos, V. Runov, A. Kepko, L. Glassmeier, K. H. Auster, H. U. McFadden, J. Carlson, C. W. Larson, D. Geophysical Research Letters Propagation characteristics of plasma sheet oscillations during a small storm General Earth and Planetary Sciences Geophysics |
| author_sort |
gabrielse, c. |
| spelling |
Gabrielse, C. Angelopoulos, V. Runov, A. Kepko, L. Glassmeier, K. H. Auster, H. U. McFadden, J. Carlson, C. W. Larson, D. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/2008gl033664 <jats:p>On 24 March 2007, the THEMIS spacecraft were in a string‐of‐pearls configuration through the dusk plasma sheet at the recovery phase of a small storm. Large undulations of the plasma sheet were observed that brought the five probes from one lobe to another. Each neutral sheet crossing was accompanied by bursty bulk flows and Pi2 oscillations. In this paper we focus on the low frequency (∼10 min) large scale plasma sheet undulations and determine their propagation characteristics, origin, and properties in the presence of storm‐time substorms. As the first case of “flapping waves” observed and analyzed during storm‐time, it is interesting to find their characteristics coincide with those described by previous quiet‐time observations. These characteristics include flankward propagation of the undulations with velocities generally between ∼40–130 km/s.</jats:p> Propagation characteristics of plasma sheet oscillations during a small storm Geophysical Research Letters |
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| title |
Propagation characteristics of plasma sheet oscillations during a small storm |
| title_unstemmed |
Propagation characteristics of plasma sheet oscillations during a small storm |
| title_full |
Propagation characteristics of plasma sheet oscillations during a small storm |
| title_fullStr |
Propagation characteristics of plasma sheet oscillations during a small storm |
| title_full_unstemmed |
Propagation characteristics of plasma sheet oscillations during a small storm |
| title_short |
Propagation characteristics of plasma sheet oscillations during a small storm |
| title_sort |
propagation characteristics of plasma sheet oscillations during a small storm |
| topic |
General Earth and Planetary Sciences Geophysics |
| url |
http://dx.doi.org/10.1029/2008gl033664 |
| publishDate |
2008 |
| physical |
|
| description |
<jats:p>On 24 March 2007, the THEMIS spacecraft were in a string‐of‐pearls configuration through the dusk plasma sheet at the recovery phase of a small storm. Large undulations of the plasma sheet were observed that brought the five probes from one lobe to another. Each neutral sheet crossing was accompanied by bursty bulk flows and Pi2 oscillations. In this paper we focus on the low frequency (∼10 min) large scale plasma sheet undulations and determine their propagation characteristics, origin, and properties in the presence of storm‐time substorms. As the first case of “flapping waves” observed and analyzed during storm‐time, it is interesting to find their characteristics coincide with those described by previous quiet‐time observations. These characteristics include flankward propagation of the undulations with velocities generally between ∼40–130 km/s.</jats:p> |
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| author | Gabrielse, C., Angelopoulos, V., Runov, A., Kepko, L., Glassmeier, K. H., Auster, H. U., McFadden, J., Carlson, C. W., Larson, D. |
| author_facet | Gabrielse, C., Angelopoulos, V., Runov, A., Kepko, L., Glassmeier, K. H., Auster, H. U., McFadden, J., Carlson, C. W., Larson, D., Gabrielse, C., Angelopoulos, V., Runov, A., Kepko, L., Glassmeier, K. H., Auster, H. U., McFadden, J., Carlson, C. W., Larson, D. |
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| description | <jats:p>On 24 March 2007, the THEMIS spacecraft were in a string‐of‐pearls configuration through the dusk plasma sheet at the recovery phase of a small storm. Large undulations of the plasma sheet were observed that brought the five probes from one lobe to another. Each neutral sheet crossing was accompanied by bursty bulk flows and Pi2 oscillations. In this paper we focus on the low frequency (∼10 min) large scale plasma sheet undulations and determine their propagation characteristics, origin, and properties in the presence of storm‐time substorms. As the first case of “flapping waves” observed and analyzed during storm‐time, it is interesting to find their characteristics coincide with those described by previous quiet‐time observations. These characteristics include flankward propagation of the undulations with velocities generally between ∼40–130 km/s.</jats:p> |
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| spelling | Gabrielse, C. Angelopoulos, V. Runov, A. Kepko, L. Glassmeier, K. H. Auster, H. U. McFadden, J. Carlson, C. W. Larson, D. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/2008gl033664 <jats:p>On 24 March 2007, the THEMIS spacecraft were in a string‐of‐pearls configuration through the dusk plasma sheet at the recovery phase of a small storm. Large undulations of the plasma sheet were observed that brought the five probes from one lobe to another. Each neutral sheet crossing was accompanied by bursty bulk flows and Pi2 oscillations. In this paper we focus on the low frequency (∼10 min) large scale plasma sheet undulations and determine their propagation characteristics, origin, and properties in the presence of storm‐time substorms. As the first case of “flapping waves” observed and analyzed during storm‐time, it is interesting to find their characteristics coincide with those described by previous quiet‐time observations. These characteristics include flankward propagation of the undulations with velocities generally between ∼40–130 km/s.</jats:p> Propagation characteristics of plasma sheet oscillations during a small storm Geophysical Research Letters |
| spellingShingle | Gabrielse, C., Angelopoulos, V., Runov, A., Kepko, L., Glassmeier, K. H., Auster, H. U., McFadden, J., Carlson, C. W., Larson, D., Geophysical Research Letters, Propagation characteristics of plasma sheet oscillations during a small storm, General Earth and Planetary Sciences, Geophysics |
| title | Propagation characteristics of plasma sheet oscillations during a small storm |
| title_full | Propagation characteristics of plasma sheet oscillations during a small storm |
| title_fullStr | Propagation characteristics of plasma sheet oscillations during a small storm |
| title_full_unstemmed | Propagation characteristics of plasma sheet oscillations during a small storm |
| title_short | Propagation characteristics of plasma sheet oscillations during a small storm |
| title_sort | propagation characteristics of plasma sheet oscillations during a small storm |
| title_unstemmed | Propagation characteristics of plasma sheet oscillations during a small storm |
| topic | General Earth and Planetary Sciences, Geophysics |
| url | http://dx.doi.org/10.1029/2008gl033664 |