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Description
| - The first (M1), second (M2), and third (M3) MESSENGER flybys of Mercury traversed the planet's magnetotail from 1.25 to 3.25 RM downstream of the planet, where RM is Mercury's radius (2440 km). The encounters took place under northward, southward, and variable-polarity interplanetary magnetic field (IMF), respectively. The magnetic field strength B in Mercury's magnetotail follows a power law decrease with increasing antisunward distance |X|, B |X|G, with G varying from -5.4 for northward to -1.6 for southward IMF. Low-latitude boundary layers (LLBLs) containing strong northward magnetic field were detected at the tail flanks during two of the flybys. The observed thickness of the LLBL was 33% and 16% of the radius of the tail during M1 and M3, respectively, but the boundary layer was completely absent during M2. Clear signatures of tail reconnection are evident in the M2 and M3 magnetic field measurements. Plasmoids and traveling compression regions were observed during M2 and M3 with typical durations of 1-3 s, suggesting diameters of 500-1500 km.
- The first (M1), second (M2), and third (M3) MESSENGER flybys of Mercury traversed the planet's magnetotail from 1.25 to 3.25 RM downstream of the planet, where RM is Mercury's radius (2440 km). The encounters took place under northward, southward, and variable-polarity interplanetary magnetic field (IMF), respectively. The magnetic field strength B in Mercury's magnetotail follows a power law decrease with increasing antisunward distance |X|, B |X|G, with G varying from -5.4 for northward to -1.6 for southward IMF. Low-latitude boundary layers (LLBLs) containing strong northward magnetic field were detected at the tail flanks during two of the flybys. The observed thickness of the LLBL was 33% and 16% of the radius of the tail during M1 and M3, respectively, but the boundary layer was completely absent during M2. Clear signatures of tail reconnection are evident in the M2 and M3 magnetic field measurements. Plasmoids and traveling compression regions were observed during M2 and M3 with typical durations of 1-3 s, suggesting diameters of 500-1500 km. (en)
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Title
| - MESSENGER and Mariner 10 flyby observations of magnetotail structure and dynamics at Mercury
- MESSENGER and Mariner 10 flyby observations of magnetotail structure and dynamics at Mercury (en)
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skos:prefLabel
| - MESSENGER and Mariner 10 flyby observations of magnetotail structure and dynamics at Mercury
- MESSENGER and Mariner 10 flyby observations of magnetotail structure and dynamics at Mercury (en)
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skos:notation
| - RIV/67985815:_____/12:00437070!RIV15-AV0-67985815
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http://linked.open...avai/riv/aktivita
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http://linked.open...avai/riv/aktivity
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http://linked.open...iv/cisloPeriodika
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http://linked.open...vai/riv/dodaniDat
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http://linked.open...aciTvurceVysledku
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http://linked.open.../riv/druhVysledku
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http://linked.open...iv/duvernostUdaju
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http://linked.open...titaPredkladatele
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http://linked.open...dnocenehoVysledku
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http://linked.open...ai/riv/idVysledku
| - RIV/67985815:_____/12:00437070
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http://linked.open...riv/jazykVysledku
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http://linked.open.../riv/klicovaSlova
| - Mercury; TCR; magnetosphere (en)
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http://linked.open.../riv/klicoveSlovo
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http://linked.open...odStatuVydavatele
| - US - Spojené státy americké
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http://linked.open...ontrolniKodProRIV
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http://linked.open...i/riv/nazevZdroje
| - Journal of Geophysical Research: Space Physics
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http://linked.open...in/vavai/riv/obor
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http://linked.open...ichTvurcuVysledku
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http://linked.open...cetTvurcuVysledku
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http://linked.open...UplatneniVysledku
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http://linked.open...v/svazekPeriodika
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http://linked.open...iv/tvurceVysledku
| - Anderson, B. J.
- Baker, D. N.
- Benna, M.
- Boardsen, S. A.
- Gold, R. E.
- Ho, G. C.
- Korth, H.
- Krimigis, S. M.
- Sarantos, M.
- Schriver, D.
- Slavin, J. A
- Trávníček, Pavel M.
- McNutt, Jr., R. L.
- Raines, J. M.
- Solomon, S. C.
- Zurbuchen, T. H.
- Imber, S.
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http://linked.open...ain/vavai/riv/wos
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issn
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number of pages
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http://bibframe.org/vocab/doi
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