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Mirror mode structures in the solar wind at 0.72 AU
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| Zeitschriftentitel: | Journal of Geophysical Research: Space Physics |
|---|---|
| Personen und Körperschaften: | , , , , , , , , , |
| In: | Journal of Geophysical Research: Space Physics, 114, 2009, A10 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
American Geophysical Union (AGU)
|
| Schlagwörter: |
| author_facet |
Zhang, T. L. Baumjohann, W. Russell, C. T. Jian, L. K. Wang, C. Cao, J. B. Balikhin, M. Blanco‐Cano, X. Delva, M. Volwerk, M. Zhang, T. L. Baumjohann, W. Russell, C. T. Jian, L. K. Wang, C. Cao, J. B. Balikhin, M. Blanco‐Cano, X. Delva, M. Volwerk, M. |
|---|---|
| author |
Zhang, T. L. Baumjohann, W. Russell, C. T. Jian, L. K. Wang, C. Cao, J. B. Balikhin, M. Blanco‐Cano, X. Delva, M. Volwerk, M. |
| spellingShingle |
Zhang, T. L. Baumjohann, W. Russell, C. T. Jian, L. K. Wang, C. Cao, J. B. Balikhin, M. Blanco‐Cano, X. Delva, M. Volwerk, M. Journal of Geophysical Research: Space Physics Mirror mode structures in the solar wind at 0.72 AU 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 |
zhang, t. l. |
| spelling |
Zhang, T. L. Baumjohann, W. Russell, C. T. Jian, L. K. Wang, C. Cao, J. B. Balikhin, M. Blanco‐Cano, X. Delva, M. Volwerk, M. 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/10.1029/2009ja014103 <jats:p>Magnetic holes in the solar wind with little or no directional change across the magnetic depression are related to mirror mode structures. Recently, Zhang et al. (2008) determined the characteristic size and shape of such mirror mode structures in the solar wind at 0.72 AU. They found that the mirror mode structure in the solar wind is quite elongated along the field direction. In this report, we examine the size and shape of isolated magnetic holes and train of holes, separately. We find that the isolated holes are slightly smaller in width and more elongated than the multiple holes. This observation suggests a particular evolutionary history of mirror mode structures in the solar wind in which multiple holes coalesce with time into isolated structures more elongated parallel to the magnetic field.</jats:p> Mirror mode structures in the solar wind at 0.72 AU Journal of Geophysical Research: Space Physics |
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Physik Technik Geologie und Paläontologie Geographie Chemie und Pharmazie Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft Biologie Allgemeine Naturwissenschaft |
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| title |
Mirror mode structures in the solar wind at 0.72 AU |
| title_unstemmed |
Mirror mode structures in the solar wind at 0.72 AU |
| title_full |
Mirror mode structures in the solar wind at 0.72 AU |
| title_fullStr |
Mirror mode structures in the solar wind at 0.72 AU |
| title_full_unstemmed |
Mirror mode structures in the solar wind at 0.72 AU |
| title_short |
Mirror mode structures in the solar wind at 0.72 AU |
| title_sort |
mirror mode structures in the solar wind at 0.72 au |
| 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/10.1029/2009ja014103 |
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2009 |
| physical |
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| description |
<jats:p>Magnetic holes in the solar wind with little or no directional change across the magnetic depression are related to mirror mode structures. Recently, Zhang et al. (2008) determined the characteristic size and shape of such mirror mode structures in the solar wind at 0.72 AU. They found that the mirror mode structure in the solar wind is quite elongated along the field direction. In this report, we examine the size and shape of isolated magnetic holes and train of holes, separately. We find that the isolated holes are slightly smaller in width and more elongated than the multiple holes. This observation suggests a particular evolutionary history of mirror mode structures in the solar wind in which multiple holes coalesce with time into isolated structures more elongated parallel to the magnetic field.</jats:p> |
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| author | Zhang, T. L., Baumjohann, W., Russell, C. T., Jian, L. K., Wang, C., Cao, J. B., Balikhin, M., Blanco‐Cano, X., Delva, M., Volwerk, M. |
| author_facet | Zhang, T. L., Baumjohann, W., Russell, C. T., Jian, L. K., Wang, C., Cao, J. B., Balikhin, M., Blanco‐Cano, X., Delva, M., Volwerk, M., Zhang, T. L., Baumjohann, W., Russell, C. T., Jian, L. K., Wang, C., Cao, J. B., Balikhin, M., Blanco‐Cano, X., Delva, M., Volwerk, M. |
| author_sort | zhang, t. l. |
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| container_title | Journal of Geophysical Research: Space Physics |
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| description | <jats:p>Magnetic holes in the solar wind with little or no directional change across the magnetic depression are related to mirror mode structures. Recently, Zhang et al. (2008) determined the characteristic size and shape of such mirror mode structures in the solar wind at 0.72 AU. They found that the mirror mode structure in the solar wind is quite elongated along the field direction. In this report, we examine the size and shape of isolated magnetic holes and train of holes, separately. We find that the isolated holes are slightly smaller in width and more elongated than the multiple holes. This observation suggests a particular evolutionary history of mirror mode structures in the solar wind in which multiple holes coalesce with time into isolated structures more elongated parallel to the magnetic field.</jats:p> |
| doi_str_mv | 10.1029/2009ja014103 |
| facet_avail | Online, Free |
| finc_class_facet | Physik, Technik, Geologie und Paläontologie, Geographie, Chemie und Pharmazie, Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft, Biologie, Allgemeine Naturwissenschaft |
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| imprint_str_mv | American Geophysical Union (AGU), 2009 |
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| series | Journal of Geophysical Research: Space Physics |
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| spelling | Zhang, T. L. Baumjohann, W. Russell, C. T. Jian, L. K. Wang, C. Cao, J. B. Balikhin, M. Blanco‐Cano, X. Delva, M. Volwerk, M. 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/10.1029/2009ja014103 <jats:p>Magnetic holes in the solar wind with little or no directional change across the magnetic depression are related to mirror mode structures. Recently, Zhang et al. (2008) determined the characteristic size and shape of such mirror mode structures in the solar wind at 0.72 AU. They found that the mirror mode structure in the solar wind is quite elongated along the field direction. In this report, we examine the size and shape of isolated magnetic holes and train of holes, separately. We find that the isolated holes are slightly smaller in width and more elongated than the multiple holes. This observation suggests a particular evolutionary history of mirror mode structures in the solar wind in which multiple holes coalesce with time into isolated structures more elongated parallel to the magnetic field.</jats:p> Mirror mode structures in the solar wind at 0.72 AU Journal of Geophysical Research: Space Physics |
| spellingShingle | Zhang, T. L., Baumjohann, W., Russell, C. T., Jian, L. K., Wang, C., Cao, J. B., Balikhin, M., Blanco‐Cano, X., Delva, M., Volwerk, M., Journal of Geophysical Research: Space Physics, Mirror mode structures in the solar wind at 0.72 AU, 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 | Mirror mode structures in the solar wind at 0.72 AU |
| title_full | Mirror mode structures in the solar wind at 0.72 AU |
| title_fullStr | Mirror mode structures in the solar wind at 0.72 AU |
| title_full_unstemmed | Mirror mode structures in the solar wind at 0.72 AU |
| title_short | Mirror mode structures in the solar wind at 0.72 AU |
| title_sort | mirror mode structures in the solar wind at 0.72 au |
| title_unstemmed | Mirror mode structures in the solar wind at 0.72 AU |
| 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/10.1029/2009ja014103 |