author_facet Lee, S. H.
Zhang, H.
Zong, Q.‐G.
Wang, Y.
Otto, A.
Rème, H.
Glassmeier, K.‐H.
Lee, S. H.
Zhang, H.
Zong, Q.‐G.
Wang, Y.
Otto, A.
Rème, H.
Glassmeier, K.‐H.
author Lee, S. H.
Zhang, H.
Zong, Q.‐G.
Wang, Y.
Otto, A.
Rème, H.
Glassmeier, K.‐H.
spellingShingle Lee, S. H.
Zhang, H.
Zong, Q.‐G.
Wang, Y.
Otto, A.
Rème, H.
Glassmeier, K.‐H.
Journal of Geophysical Research: Space Physics
Asymmetric ionospheric outflow observed at the dayside magnetopause
Space and Planetary Science
Geophysics
author_sort lee, s. h.
spelling Lee, S. H. Zhang, H. Zong, Q.‐G. Wang, Y. Otto, A. Rème, H. Glassmeier, K.‐H. 2169-9380 2169-9402 American Geophysical Union (AGU) Space and Planetary Science Geophysics http://dx.doi.org/10.1002/2014ja020943 <jats:title>Abstract</jats:title><jats:p>An important source of the terrestrial magnetospheric plasma is the Earth's ionospheric outflows from the high‐latitude regions of both hemispheres. The ionospheric ion outflows have rarely been observed at the dayside magnetopause. We report Cluster observations of the ionospheric ion outflows observed at the dayside magnetopause. The low‐energy (up to 1.5 keV) electrons are detected with bidirectional pitch angle distributions indicating that the magnetic field lines are closed. The unidirectional cold ions (&lt; 200 eV) are observed in the magnetosphere by both C1 and C3. The pitch angle distributions (0<jats:sup>∘</jats:sup>–75<jats:sup>∘</jats:sup>) of the cold ions (&lt; 1 keV) at the dayside magnetopause indicate that these cold ions are the ionospheric outflows coming only from the Southern Hemisphere. The cold ions (&lt; 200 eV) fluxes are modulated by the ULF wave electric field. Two different species (possibly H<jats:sup>+</jats:sup> and He<jats:sup>+</jats:sup>) are observed in the magnetosphere. Our results suggest that the ionospheric outflows can directly reach the dayside magnetopause region and may participate in the reconnection process.</jats:p> Asymmetric ionospheric outflow observed at the dayside magnetopause Journal of Geophysical Research: Space Physics
doi_str_mv 10.1002/2014ja020943
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recordtype ai
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series Journal of Geophysical Research: Space Physics
source_id 49
title Asymmetric ionospheric outflow observed at the dayside magnetopause
title_unstemmed Asymmetric ionospheric outflow observed at the dayside magnetopause
title_full Asymmetric ionospheric outflow observed at the dayside magnetopause
title_fullStr Asymmetric ionospheric outflow observed at the dayside magnetopause
title_full_unstemmed Asymmetric ionospheric outflow observed at the dayside magnetopause
title_short Asymmetric ionospheric outflow observed at the dayside magnetopause
title_sort asymmetric ionospheric outflow observed at the dayside magnetopause
topic Space and Planetary Science
Geophysics
url http://dx.doi.org/10.1002/2014ja020943
publishDate 2015
physical 3564-3573
description <jats:title>Abstract</jats:title><jats:p>An important source of the terrestrial magnetospheric plasma is the Earth's ionospheric outflows from the high‐latitude regions of both hemispheres. The ionospheric ion outflows have rarely been observed at the dayside magnetopause. We report Cluster observations of the ionospheric ion outflows observed at the dayside magnetopause. The low‐energy (up to 1.5 keV) electrons are detected with bidirectional pitch angle distributions indicating that the magnetic field lines are closed. The unidirectional cold ions (&lt; 200 eV) are observed in the magnetosphere by both C1 and C3. The pitch angle distributions (0<jats:sup>∘</jats:sup>–75<jats:sup>∘</jats:sup>) of the cold ions (&lt; 1 keV) at the dayside magnetopause indicate that these cold ions are the ionospheric outflows coming only from the Southern Hemisphere. The cold ions (&lt; 200 eV) fluxes are modulated by the ULF wave electric field. Two different species (possibly H<jats:sup>+</jats:sup> and He<jats:sup>+</jats:sup>) are observed in the magnetosphere. Our results suggest that the ionospheric outflows can directly reach the dayside magnetopause region and may participate in the reconnection process.</jats:p>
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author Lee, S. H., Zhang, H., Zong, Q.‐G., Wang, Y., Otto, A., Rème, H., Glassmeier, K.‐H.
author_facet Lee, S. H., Zhang, H., Zong, Q.‐G., Wang, Y., Otto, A., Rème, H., Glassmeier, K.‐H., Lee, S. H., Zhang, H., Zong, Q.‐G., Wang, Y., Otto, A., Rème, H., Glassmeier, K.‐H.
author_sort lee, s. h.
container_issue 5
container_start_page 3564
container_title Journal of Geophysical Research: Space Physics
container_volume 120
description <jats:title>Abstract</jats:title><jats:p>An important source of the terrestrial magnetospheric plasma is the Earth's ionospheric outflows from the high‐latitude regions of both hemispheres. The ionospheric ion outflows have rarely been observed at the dayside magnetopause. We report Cluster observations of the ionospheric ion outflows observed at the dayside magnetopause. The low‐energy (up to 1.5 keV) electrons are detected with bidirectional pitch angle distributions indicating that the magnetic field lines are closed. The unidirectional cold ions (&lt; 200 eV) are observed in the magnetosphere by both C1 and C3. The pitch angle distributions (0<jats:sup>∘</jats:sup>–75<jats:sup>∘</jats:sup>) of the cold ions (&lt; 1 keV) at the dayside magnetopause indicate that these cold ions are the ionospheric outflows coming only from the Southern Hemisphere. The cold ions (&lt; 200 eV) fluxes are modulated by the ULF wave electric field. Two different species (possibly H<jats:sup>+</jats:sup> and He<jats:sup>+</jats:sup>) are observed in the magnetosphere. Our results suggest that the ionospheric outflows can directly reach the dayside magnetopause region and may participate in the reconnection process.</jats:p>
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spelling Lee, S. H. Zhang, H. Zong, Q.‐G. Wang, Y. Otto, A. Rème, H. Glassmeier, K.‐H. 2169-9380 2169-9402 American Geophysical Union (AGU) Space and Planetary Science Geophysics http://dx.doi.org/10.1002/2014ja020943 <jats:title>Abstract</jats:title><jats:p>An important source of the terrestrial magnetospheric plasma is the Earth's ionospheric outflows from the high‐latitude regions of both hemispheres. The ionospheric ion outflows have rarely been observed at the dayside magnetopause. We report Cluster observations of the ionospheric ion outflows observed at the dayside magnetopause. The low‐energy (up to 1.5 keV) electrons are detected with bidirectional pitch angle distributions indicating that the magnetic field lines are closed. The unidirectional cold ions (&lt; 200 eV) are observed in the magnetosphere by both C1 and C3. The pitch angle distributions (0<jats:sup>∘</jats:sup>–75<jats:sup>∘</jats:sup>) of the cold ions (&lt; 1 keV) at the dayside magnetopause indicate that these cold ions are the ionospheric outflows coming only from the Southern Hemisphere. The cold ions (&lt; 200 eV) fluxes are modulated by the ULF wave electric field. Two different species (possibly H<jats:sup>+</jats:sup> and He<jats:sup>+</jats:sup>) are observed in the magnetosphere. Our results suggest that the ionospheric outflows can directly reach the dayside magnetopause region and may participate in the reconnection process.</jats:p> Asymmetric ionospheric outflow observed at the dayside magnetopause Journal of Geophysical Research: Space Physics
spellingShingle Lee, S. H., Zhang, H., Zong, Q.‐G., Wang, Y., Otto, A., Rème, H., Glassmeier, K.‐H., Journal of Geophysical Research: Space Physics, Asymmetric ionospheric outflow observed at the dayside magnetopause, Space and Planetary Science, Geophysics
title Asymmetric ionospheric outflow observed at the dayside magnetopause
title_full Asymmetric ionospheric outflow observed at the dayside magnetopause
title_fullStr Asymmetric ionospheric outflow observed at the dayside magnetopause
title_full_unstemmed Asymmetric ionospheric outflow observed at the dayside magnetopause
title_short Asymmetric ionospheric outflow observed at the dayside magnetopause
title_sort asymmetric ionospheric outflow observed at the dayside magnetopause
title_unstemmed Asymmetric ionospheric outflow observed at the dayside magnetopause
topic Space and Planetary Science, Geophysics
url http://dx.doi.org/10.1002/2014ja020943