author_facet Kawano, H.
Russell, C. T.
Kawano, H.
Russell, C. T.
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> &lt; 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> &gt; 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
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Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft
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Geologie und Paläontologie
Geographie
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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> &lt; 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> &gt; 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> &lt; 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> &gt; 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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finc_class_facet Chemie und Pharmazie, Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft, Biologie, Allgemeine Naturwissenschaft, Physik, Technik, Geologie und Paläontologie, Geographie
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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> &lt; 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> &gt; 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