A multi-scale magnetotail reconnection event at Saturn and associated flows: Cassini/UVIS observations
UVIS/Cassini reveals enhanced dawn auroral activity at Saturn. * The auroral dawn enhancement is suggested to be related to magnetotail reconnection. * The observations suggest an x-line which extends from 02 to 05LT. * Arc and spot-like small scale features are possibly related to plasma flows.
Gespeichert in:
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Radioti, A [verfasserIn] |
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Artikel |
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Englisch |
| Erschienen: |
2016 |
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| Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Icarus - Amsterdam [u.a.] : Elsevier, 1962, 263(2016), Seite 75-82 |
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| Übergeordnetes Werk: |
volume:263 ; year:2016 ; pages:75-82 |
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| DOI / URN: |
10.1016/j.icarus.2014.12.016 |
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| 520 | |a UVIS/Cassini reveals enhanced dawn auroral activity at Saturn. * The auroral dawn enhancement is suggested to be related to magnetotail reconnection. * The observations suggest an x-line which extends from 02 to 05LT. * Arc and spot-like small scale features are possibly related to plasma flows. | ||
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A multi-scale magnetotail reconnection event at Saturn and associated flows: Cassini/UVIS observations |
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UVIS/Cassini reveals enhanced dawn auroral activity at Saturn. * The auroral dawn enhancement is suggested to be related to magnetotail reconnection. * The observations suggest an x-line which extends from 02 to 05LT. * Arc and spot-like small scale features are possibly related to plasma flows. |
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UVIS/Cassini reveals enhanced dawn auroral activity at Saturn. * The auroral dawn enhancement is suggested to be related to magnetotail reconnection. * The observations suggest an x-line which extends from 02 to 05LT. * Arc and spot-like small scale features are possibly related to plasma flows. |
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UVIS/Cassini reveals enhanced dawn auroral activity at Saturn. * The auroral dawn enhancement is suggested to be related to magnetotail reconnection. * The observations suggest an x-line which extends from 02 to 05LT. * Arc and spot-like small scale features are possibly related to plasma flows. |
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A multi-scale magnetotail reconnection event at Saturn and associated flows: Cassini/UVIS observations |
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10.1016/j.icarus.2014.12.016 |
| up_date |
2024-07-03T15:24:43.731Z |
| _version_ |
1803571989030371328 |
| fullrecord_marcxml |
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7.3991003 |