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Cause of postterminator flux transfer events
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Zeitschriftentitel: | Journal of Geophysical Research: Space Physics |
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Personen und Körperschaften: | , |
In: | Journal of Geophysical Research: Space Physics, 102, 1997, A12, S. 27029-27038 |
Format: | E-Article |
Sprache: | Englisch |
veröffentlicht: |
American Geophysical Union (AGU)
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Schlagwörter: |
author_facet |
Kawano, H. Russell, C. T. Kawano, H. Russell, C. T. |
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author |
Kawano, H. Russell, C. T. |
spellingShingle |
Kawano, H. Russell, C. T. Journal of Geophysical Research: Space Physics Cause of postterminator flux transfer events Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics |
author_sort |
kawano, h. |
spelling |
Kawano, H. Russell, C. T. 0148-0227 American Geophysical Union (AGU) Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics http://dx.doi.org/10.1029/97ja02139 <jats:p>The local time at which flux transfer events (FTEs) are observed affects the interplanetary magnetic field (IMF) dependence of their occurrence [<jats:italic>Kawano and Russell</jats:italic>, 1997]. Subsolar FTEs occur mainly during southward IMF, consistent with the day side reconnection model. Postterminator FTEs occur during both southward and northward IMF but are not simply generated by pressure pulses convected to the magnetopause from the foreshock. This paper evaluates other possible generation mechanisms of these postterminator FTEs. We attribute the generation of the postterminator FTEs when IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> < 0 to an “equatorial reconnection line,” which is tilted according to the IMF <jats:italic>B<jats:sub>y</jats:sub></jats:italic>, just as we do for subsolar FTEs. When IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> > 0, we find it unlikely that the postterminator FTEs are generated by local reconnection. Two possible sources are cusp reconnection and the “equatorial reconnection,” with re‐reconnection in the subsolar region [<jats:italic>Nishida</jats:italic>, 1989]. When the IMF is northerly directed but mostly equatorial, the “equatorial reconnection line” model fits better with observations. When the IMF is more northward, both models can explain observations we have at hand.</jats:p> Cause of postterminator flux transfer events Journal of Geophysical Research: Space Physics |
doi_str_mv |
10.1029/97ja02139 |
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Online Free |
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Chemie und Pharmazie Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft Biologie Allgemeine Naturwissenschaft Physik Technik Geologie und Paläontologie Geographie |
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American Geophysical Union (AGU), 1997 |
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Journal of Geophysical Research: Space Physics |
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title |
Cause of postterminator flux transfer events |
title_unstemmed |
Cause of postterminator flux transfer events |
title_full |
Cause of postterminator flux transfer events |
title_fullStr |
Cause of postterminator flux transfer events |
title_full_unstemmed |
Cause of postterminator flux transfer events |
title_short |
Cause of postterminator flux transfer events |
title_sort |
cause of postterminator flux transfer events |
topic |
Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics |
url |
http://dx.doi.org/10.1029/97ja02139 |
publishDate |
1997 |
physical |
27029-27038 |
description |
<jats:p>The local time at which flux transfer events (FTEs) are observed affects the interplanetary magnetic field (IMF) dependence of their occurrence [<jats:italic>Kawano and Russell</jats:italic>, 1997]. Subsolar FTEs occur mainly during southward IMF, consistent with the day side reconnection model. Postterminator FTEs occur during both southward and northward IMF but are not simply generated by pressure pulses convected to the magnetopause from the foreshock. This paper evaluates other possible generation mechanisms of these postterminator FTEs. We attribute the generation of the postterminator FTEs when IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> < 0 to an “equatorial reconnection line,” which is tilted according to the IMF <jats:italic>B<jats:sub>y</jats:sub></jats:italic>, just as we do for subsolar FTEs. When IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> > 0, we find it unlikely that the postterminator FTEs are generated by local reconnection. Two possible sources are cusp reconnection and the “equatorial reconnection,” with re‐reconnection in the subsolar region [<jats:italic>Nishida</jats:italic>, 1989]. When the IMF is northerly directed but mostly equatorial, the “equatorial reconnection line” model fits better with observations. When the IMF is more northward, both models can explain observations we have at hand.</jats:p> |
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author | Kawano, H., Russell, C. T. |
author_facet | Kawano, H., Russell, C. T., Kawano, H., Russell, C. T. |
author_sort | kawano, h. |
container_issue | A12 |
container_start_page | 27029 |
container_title | Journal of Geophysical Research: Space Physics |
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description | <jats:p>The local time at which flux transfer events (FTEs) are observed affects the interplanetary magnetic field (IMF) dependence of their occurrence [<jats:italic>Kawano and Russell</jats:italic>, 1997]. Subsolar FTEs occur mainly during southward IMF, consistent with the day side reconnection model. Postterminator FTEs occur during both southward and northward IMF but are not simply generated by pressure pulses convected to the magnetopause from the foreshock. This paper evaluates other possible generation mechanisms of these postterminator FTEs. We attribute the generation of the postterminator FTEs when IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> < 0 to an “equatorial reconnection line,” which is tilted according to the IMF <jats:italic>B<jats:sub>y</jats:sub></jats:italic>, just as we do for subsolar FTEs. When IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> > 0, we find it unlikely that the postterminator FTEs are generated by local reconnection. Two possible sources are cusp reconnection and the “equatorial reconnection,” with re‐reconnection in the subsolar region [<jats:italic>Nishida</jats:italic>, 1989]. When the IMF is northerly directed but mostly equatorial, the “equatorial reconnection line” model fits better with observations. When the IMF is more northward, both models can explain observations we have at hand.</jats:p> |
doi_str_mv | 10.1029/97ja02139 |
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physical | 27029-27038 |
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publisher | American Geophysical Union (AGU) |
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series | Journal of Geophysical Research: Space Physics |
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spelling | Kawano, H. Russell, C. T. 0148-0227 American Geophysical Union (AGU) Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics http://dx.doi.org/10.1029/97ja02139 <jats:p>The local time at which flux transfer events (FTEs) are observed affects the interplanetary magnetic field (IMF) dependence of their occurrence [<jats:italic>Kawano and Russell</jats:italic>, 1997]. Subsolar FTEs occur mainly during southward IMF, consistent with the day side reconnection model. Postterminator FTEs occur during both southward and northward IMF but are not simply generated by pressure pulses convected to the magnetopause from the foreshock. This paper evaluates other possible generation mechanisms of these postterminator FTEs. We attribute the generation of the postterminator FTEs when IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> < 0 to an “equatorial reconnection line,” which is tilted according to the IMF <jats:italic>B<jats:sub>y</jats:sub></jats:italic>, just as we do for subsolar FTEs. When IMF <jats:italic>B<jats:sub>z</jats:sub></jats:italic> > 0, we find it unlikely that the postterminator FTEs are generated by local reconnection. Two possible sources are cusp reconnection and the “equatorial reconnection,” with re‐reconnection in the subsolar region [<jats:italic>Nishida</jats:italic>, 1989]. When the IMF is northerly directed but mostly equatorial, the “equatorial reconnection line” model fits better with observations. When the IMF is more northward, both models can explain observations we have at hand.</jats:p> Cause of postterminator flux transfer events Journal of Geophysical Research: Space Physics |
spellingShingle | Kawano, H., Russell, C. T., Journal of Geophysical Research: Space Physics, Cause of postterminator flux transfer events, Paleontology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Earth-Surface Processes, Geochemistry and Petrology, Soil Science, Water Science and Technology, Ecology, Aquatic Science, Forestry, Oceanography, Geophysics |
title | Cause of postterminator flux transfer events |
title_full | Cause of postterminator flux transfer events |
title_fullStr | Cause of postterminator flux transfer events |
title_full_unstemmed | Cause of postterminator flux transfer events |
title_short | Cause of postterminator flux transfer events |
title_sort | cause of postterminator flux transfer events |
title_unstemmed | Cause of postterminator flux transfer events |
topic | Paleontology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Earth-Surface Processes, Geochemistry and Petrology, Soil Science, Water Science and Technology, Ecology, Aquatic Science, Forestry, Oceanography, Geophysics |
url | http://dx.doi.org/10.1029/97ja02139 |