author_facet Teh, W.‐L.
Nakamura, R.
Baumjohann, W.
Teh, W.‐L.
Nakamura, R.
Baumjohann, W.
author Teh, W.‐L.
Nakamura, R.
Baumjohann, W.
spellingShingle Teh, W.‐L.
Nakamura, R.
Baumjohann, W.
Journal of Geophysical Research: Space Physics
Magnetic field topology of the plasma sheet boundary layer
Space and Planetary Science
Geophysics
author_sort teh, w.‐l.
spelling Teh, W.‐L. Nakamura, R. Baumjohann, W. 2169-9380 2169-9402 American Geophysical Union (AGU) Space and Planetary Science Geophysics http://dx.doi.org/10.1002/jgra.50435 <jats:title>Abstract</jats:title><jats:p>The magnetic field topology of the plasma sheet boundary layer (PSBL) and its neighborhood is examined using a steady, two‐dimensional (2‐D), ideal MHD reconstruction method. We study four PSBL crossings, from the lobe toward the plasma sheet and back into the lobe, by the Cluster spacecraft in the Earth's magnetotail around (x, y, z) = (–17.3, 4.3, –6.3) R<jats:sub>E</jats:sub> in GSM. The four PSBL events are selected for having no intense ion beams. Two reconstructed magnetic field topologies give, for the first time, a 3‐D view of the PSBL, showing that one has a rather large gradient in the magnetic structure than another. A quantitative agreement of the current density between the reconstruction and curlometer methods is achieved for the overall results but with some discrepancies remaining, which will be discussed in terms of 3‐D and temporal effects. This agreement indicates that the current density can be estimated by the reconstruction if certain conditions are satisfied. Finally, we point out that a PSBL structure with intense ion beams would somehow degrade the accuracy of the ideal MHD reconstruction. This degradation may be due to the nonideal MHD properties and/or the transient properties of the ion beams. Further sophisticated investigations on this issue are needed for clarification.</jats:p> Magnetic field topology of the plasma sheet boundary layer Journal of Geophysical Research: Space Physics
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series Journal of Geophysical Research: Space Physics
source_id 49
title Magnetic field topology of the plasma sheet boundary layer
title_unstemmed Magnetic field topology of the plasma sheet boundary layer
title_full Magnetic field topology of the plasma sheet boundary layer
title_fullStr Magnetic field topology of the plasma sheet boundary layer
title_full_unstemmed Magnetic field topology of the plasma sheet boundary layer
title_short Magnetic field topology of the plasma sheet boundary layer
title_sort magnetic field topology of the plasma sheet boundary layer
topic Space and Planetary Science
Geophysics
url http://dx.doi.org/10.1002/jgra.50435
publishDate 2013
physical 4059-4065
description <jats:title>Abstract</jats:title><jats:p>The magnetic field topology of the plasma sheet boundary layer (PSBL) and its neighborhood is examined using a steady, two‐dimensional (2‐D), ideal MHD reconstruction method. We study four PSBL crossings, from the lobe toward the plasma sheet and back into the lobe, by the Cluster spacecraft in the Earth's magnetotail around (x, y, z) = (–17.3, 4.3, –6.3) R<jats:sub>E</jats:sub> in GSM. The four PSBL events are selected for having no intense ion beams. Two reconstructed magnetic field topologies give, for the first time, a 3‐D view of the PSBL, showing that one has a rather large gradient in the magnetic structure than another. A quantitative agreement of the current density between the reconstruction and curlometer methods is achieved for the overall results but with some discrepancies remaining, which will be discussed in terms of 3‐D and temporal effects. This agreement indicates that the current density can be estimated by the reconstruction if certain conditions are satisfied. Finally, we point out that a PSBL structure with intense ion beams would somehow degrade the accuracy of the ideal MHD reconstruction. This degradation may be due to the nonideal MHD properties and/or the transient properties of the ion beams. Further sophisticated investigations on this issue are needed for clarification.</jats:p>
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author Teh, W.‐L., Nakamura, R., Baumjohann, W.
author_facet Teh, W.‐L., Nakamura, R., Baumjohann, W., Teh, W.‐L., Nakamura, R., Baumjohann, W.
author_sort teh, w.‐l.
container_issue 7
container_start_page 4059
container_title Journal of Geophysical Research: Space Physics
container_volume 118
description <jats:title>Abstract</jats:title><jats:p>The magnetic field topology of the plasma sheet boundary layer (PSBL) and its neighborhood is examined using a steady, two‐dimensional (2‐D), ideal MHD reconstruction method. We study four PSBL crossings, from the lobe toward the plasma sheet and back into the lobe, by the Cluster spacecraft in the Earth's magnetotail around (x, y, z) = (–17.3, 4.3, –6.3) R<jats:sub>E</jats:sub> in GSM. The four PSBL events are selected for having no intense ion beams. Two reconstructed magnetic field topologies give, for the first time, a 3‐D view of the PSBL, showing that one has a rather large gradient in the magnetic structure than another. A quantitative agreement of the current density between the reconstruction and curlometer methods is achieved for the overall results but with some discrepancies remaining, which will be discussed in terms of 3‐D and temporal effects. This agreement indicates that the current density can be estimated by the reconstruction if certain conditions are satisfied. Finally, we point out that a PSBL structure with intense ion beams would somehow degrade the accuracy of the ideal MHD reconstruction. This degradation may be due to the nonideal MHD properties and/or the transient properties of the ion beams. Further sophisticated investigations on this issue are needed for clarification.</jats:p>
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imprint_str_mv American Geophysical Union (AGU), 2013
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spelling Teh, W.‐L. Nakamura, R. Baumjohann, W. 2169-9380 2169-9402 American Geophysical Union (AGU) Space and Planetary Science Geophysics http://dx.doi.org/10.1002/jgra.50435 <jats:title>Abstract</jats:title><jats:p>The magnetic field topology of the plasma sheet boundary layer (PSBL) and its neighborhood is examined using a steady, two‐dimensional (2‐D), ideal MHD reconstruction method. We study four PSBL crossings, from the lobe toward the plasma sheet and back into the lobe, by the Cluster spacecraft in the Earth's magnetotail around (x, y, z) = (–17.3, 4.3, –6.3) R<jats:sub>E</jats:sub> in GSM. The four PSBL events are selected for having no intense ion beams. Two reconstructed magnetic field topologies give, for the first time, a 3‐D view of the PSBL, showing that one has a rather large gradient in the magnetic structure than another. A quantitative agreement of the current density between the reconstruction and curlometer methods is achieved for the overall results but with some discrepancies remaining, which will be discussed in terms of 3‐D and temporal effects. This agreement indicates that the current density can be estimated by the reconstruction if certain conditions are satisfied. Finally, we point out that a PSBL structure with intense ion beams would somehow degrade the accuracy of the ideal MHD reconstruction. This degradation may be due to the nonideal MHD properties and/or the transient properties of the ion beams. Further sophisticated investigations on this issue are needed for clarification.</jats:p> Magnetic field topology of the plasma sheet boundary layer Journal of Geophysical Research: Space Physics
spellingShingle Teh, W.‐L., Nakamura, R., Baumjohann, W., Journal of Geophysical Research: Space Physics, Magnetic field topology of the plasma sheet boundary layer, Space and Planetary Science, Geophysics
title Magnetic field topology of the plasma sheet boundary layer
title_full Magnetic field topology of the plasma sheet boundary layer
title_fullStr Magnetic field topology of the plasma sheet boundary layer
title_full_unstemmed Magnetic field topology of the plasma sheet boundary layer
title_short Magnetic field topology of the plasma sheet boundary layer
title_sort magnetic field topology of the plasma sheet boundary layer
title_unstemmed Magnetic field topology of the plasma sheet boundary layer
topic Space and Planetary Science, Geophysics
url http://dx.doi.org/10.1002/jgra.50435