author_facet Keika, K.
Nakamura, R.
Baumjohann, W.
Angelopoulos, V.
Chi, P. J.
Glassmeier, K. H.
Fillingim, M.
Magnes, W.
Auster, H. U.
Fornaçon, K. H.
Reeves, G. D.
Yumoto, K.
Lucek, E. A.
Carr, C. M.
Dandouras, I.
Keika, K.
Nakamura, R.
Baumjohann, W.
Angelopoulos, V.
Chi, P. J.
Glassmeier, K. H.
Fillingim, M.
Magnes, W.
Auster, H. U.
Fornaçon, K. H.
Reeves, G. D.
Yumoto, K.
Lucek, E. A.
Carr, C. M.
Dandouras, I.
author Keika, K.
Nakamura, R.
Baumjohann, W.
Angelopoulos, V.
Chi, P. J.
Glassmeier, K. H.
Fillingim, M.
Magnes, W.
Auster, H. U.
Fornaçon, K. H.
Reeves, G. D.
Yumoto, K.
Lucek, E. A.
Carr, C. M.
Dandouras, I.
spellingShingle Keika, K.
Nakamura, R.
Baumjohann, W.
Angelopoulos, V.
Chi, P. J.
Glassmeier, K. H.
Fillingim, M.
Magnes, W.
Auster, H. U.
Fornaçon, K. H.
Reeves, G. D.
Yumoto, K.
Lucek, E. A.
Carr, C. M.
Dandouras, I.
Journal of Geophysical Research: Space Physics
Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
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 keika, k.
spelling Keika, K. Nakamura, R. Baumjohann, W. Angelopoulos, V. Chi, P. J. Glassmeier, K. H. Fillingim, M. Magnes, W. Auster, H. U. Fornaçon, K. H. Reeves, G. D. Yumoto, K. Lucek, E. A. Carr, C. M. Dandouras, I. 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/10.1029/2008ja013445 <jats:p>We examine a substorm expansion on 21 June 2007, which occurred &lt;2 min after a solar wind discontinuity accompanied by a dynamic pressure (<jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub>) increase impinged on the magnetopause. To investigate how the perturbation due to such <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase propagates in the magnetosphere and what the timing analysis may imply about how this type of substorms is triggered, we utilize a large number of in situ magnetic field and plasma observations, a remote sensing of auroral brightening, and ground‐based magnetic field observations. The timing analysis shows that the front of a compression‐associated sudden impulse can reach the substorm expansion onset site (dawnside near‐Earth plasma sheet) at the substorm onset time. The onset site and time are determined from aurora images displaying aurora expansion, energetic electron data at geosynchronous orbit showing dispersed injection, and geomagnetic field data at high latitudes showing negative bays in the <jats:italic>H</jats:italic> component. Our 2‐D calculations of the fast‐mode propagation also demonstrate the arrival of the wavefront at the onset site and time. We suggest that for the class of substorms triggered by solar wind <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increases, the triggering could occur within as short as 2 min after a <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase impinges on the magnetopause, consistent with the time needed for the sudden impulse wavefront to propagate inside the magnetosphere from the dayside magnetopause to the magnetotail.</jats:p> Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause Journal of Geophysical Research: Space Physics
doi_str_mv 10.1029/2008ja013445
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Chemie und Pharmazie
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series Journal of Geophysical Research: Space Physics
source_id 49
title Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_unstemmed Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_full Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_fullStr Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_full_unstemmed Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_short Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_sort substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
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/10.1029/2008ja013445
publishDate 2009
physical
description <jats:p>We examine a substorm expansion on 21 June 2007, which occurred &lt;2 min after a solar wind discontinuity accompanied by a dynamic pressure (<jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub>) increase impinged on the magnetopause. To investigate how the perturbation due to such <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase propagates in the magnetosphere and what the timing analysis may imply about how this type of substorms is triggered, we utilize a large number of in situ magnetic field and plasma observations, a remote sensing of auroral brightening, and ground‐based magnetic field observations. The timing analysis shows that the front of a compression‐associated sudden impulse can reach the substorm expansion onset site (dawnside near‐Earth plasma sheet) at the substorm onset time. The onset site and time are determined from aurora images displaying aurora expansion, energetic electron data at geosynchronous orbit showing dispersed injection, and geomagnetic field data at high latitudes showing negative bays in the <jats:italic>H</jats:italic> component. Our 2‐D calculations of the fast‐mode propagation also demonstrate the arrival of the wavefront at the onset site and time. We suggest that for the class of substorms triggered by solar wind <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increases, the triggering could occur within as short as 2 min after a <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase impinges on the magnetopause, consistent with the time needed for the sudden impulse wavefront to propagate inside the magnetosphere from the dayside magnetopause to the magnetotail.</jats:p>
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author Keika, K., Nakamura, R., Baumjohann, W., Angelopoulos, V., Chi, P. J., Glassmeier, K. H., Fillingim, M., Magnes, W., Auster, H. U., Fornaçon, K. H., Reeves, G. D., Yumoto, K., Lucek, E. A., Carr, C. M., Dandouras, I.
author_facet Keika, K., Nakamura, R., Baumjohann, W., Angelopoulos, V., Chi, P. J., Glassmeier, K. H., Fillingim, M., Magnes, W., Auster, H. U., Fornaçon, K. H., Reeves, G. D., Yumoto, K., Lucek, E. A., Carr, C. M., Dandouras, I., Keika, K., Nakamura, R., Baumjohann, W., Angelopoulos, V., Chi, P. J., Glassmeier, K. H., Fillingim, M., Magnes, W., Auster, H. U., Fornaçon, K. H., Reeves, G. D., Yumoto, K., Lucek, E. A., Carr, C. M., Dandouras, I.
author_sort keika, k.
container_issue A1
container_start_page 0
container_title Journal of Geophysical Research: Space Physics
container_volume 114
description <jats:p>We examine a substorm expansion on 21 June 2007, which occurred &lt;2 min after a solar wind discontinuity accompanied by a dynamic pressure (<jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub>) increase impinged on the magnetopause. To investigate how the perturbation due to such <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase propagates in the magnetosphere and what the timing analysis may imply about how this type of substorms is triggered, we utilize a large number of in situ magnetic field and plasma observations, a remote sensing of auroral brightening, and ground‐based magnetic field observations. The timing analysis shows that the front of a compression‐associated sudden impulse can reach the substorm expansion onset site (dawnside near‐Earth plasma sheet) at the substorm onset time. The onset site and time are determined from aurora images displaying aurora expansion, energetic electron data at geosynchronous orbit showing dispersed injection, and geomagnetic field data at high latitudes showing negative bays in the <jats:italic>H</jats:italic> component. Our 2‐D calculations of the fast‐mode propagation also demonstrate the arrival of the wavefront at the onset site and time. We suggest that for the class of substorms triggered by solar wind <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increases, the triggering could occur within as short as 2 min after a <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase impinges on the magnetopause, consistent with the time needed for the sudden impulse wavefront to propagate inside the magnetosphere from the dayside magnetopause to the magnetotail.</jats:p>
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spelling Keika, K. Nakamura, R. Baumjohann, W. Angelopoulos, V. Chi, P. J. Glassmeier, K. H. Fillingim, M. Magnes, W. Auster, H. U. Fornaçon, K. H. Reeves, G. D. Yumoto, K. Lucek, E. A. Carr, C. M. Dandouras, I. 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/10.1029/2008ja013445 <jats:p>We examine a substorm expansion on 21 June 2007, which occurred &lt;2 min after a solar wind discontinuity accompanied by a dynamic pressure (<jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub>) increase impinged on the magnetopause. To investigate how the perturbation due to such <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase propagates in the magnetosphere and what the timing analysis may imply about how this type of substorms is triggered, we utilize a large number of in situ magnetic field and plasma observations, a remote sensing of auroral brightening, and ground‐based magnetic field observations. The timing analysis shows that the front of a compression‐associated sudden impulse can reach the substorm expansion onset site (dawnside near‐Earth plasma sheet) at the substorm onset time. The onset site and time are determined from aurora images displaying aurora expansion, energetic electron data at geosynchronous orbit showing dispersed injection, and geomagnetic field data at high latitudes showing negative bays in the <jats:italic>H</jats:italic> component. Our 2‐D calculations of the fast‐mode propagation also demonstrate the arrival of the wavefront at the onset site and time. We suggest that for the class of substorms triggered by solar wind <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increases, the triggering could occur within as short as 2 min after a <jats:italic>P</jats:italic><jats:sub><jats:italic>d</jats:italic></jats:sub> increase impinges on the magnetopause, consistent with the time needed for the sudden impulse wavefront to propagate inside the magnetosphere from the dayside magnetopause to the magnetotail.</jats:p> Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause Journal of Geophysical Research: Space Physics
spellingShingle Keika, K., Nakamura, R., Baumjohann, W., Angelopoulos, V., Chi, P. J., Glassmeier, K. H., Fillingim, M., Magnes, W., Auster, H. U., Fornaçon, K. H., Reeves, G. D., Yumoto, K., Lucek, E. A., Carr, C. M., Dandouras, I., Journal of Geophysical Research: Space Physics, Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause, 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 Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_full Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_fullStr Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_full_unstemmed Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_short Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_sort substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
title_unstemmed Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause
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/10.1029/2008ja013445