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Cassini in situ observations of long-duration magnetic reconnection in Saturn’s magnetotail
by
André, N.
, Kidder, A.
, Volwerk, M.
, Lamy, L.
, Sergis, N.
, Poh, G.-K.
, Jia, X.
, Coates, A. J.
, Thomsen, M. F.
, Dougherty, M. K.
, Jackman, C. M.
, Slavin, J. A.
, Arridge, C. S.
, Walsh, A. P.
, Eastwood, J. P.
, Zarka, P.
, Radioti, A.
, Reisenfeld, D. B.
in
639/33/445/846
/ 639/33/525/869
/ 639/766/1960
/ Astrophysics
/ Atomic
/ Aérospatiale, astronomie & astrophysique
/ Cassini mission
/ Classical and Continuum Physics
/ Complex Systems
/ Condensed Matter Physics
/ Current sheets
/ Diffusion
/ Jupiter
/ Jupiter (planet)
/ Kinetics
/ letter
/ Magnetic fields
/ Magnetism
/ Magnetospheres
/ Magnetotails
/ Mathematical and Computational Physics
/ Molecular
/ Optical and Plasma Physics
/ Physical, chemical, mathematical & earth Sciences
/ Physics
/ Physique, chimie, mathématiques & sciences de la terre
/ Planetary magnetospheres
/ Plasma
/ Plasma loss
/ Plasmas
/ Reconfiguration
/ Rotating bodies
/ Rotation
/ Saturn
/ Saturn (planet)
/ Solar system
/ Space science, astronomy & astrophysics
/ Spacecraft
/ Theoretical
/ Wave energy
2016
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Cassini in situ observations of long-duration magnetic reconnection in Saturn’s magnetotail
by
André, N.
, Kidder, A.
, Volwerk, M.
, Lamy, L.
, Sergis, N.
, Poh, G.-K.
, Jia, X.
, Coates, A. J.
, Thomsen, M. F.
, Dougherty, M. K.
, Jackman, C. M.
, Slavin, J. A.
, Arridge, C. S.
, Walsh, A. P.
, Eastwood, J. P.
, Zarka, P.
, Radioti, A.
, Reisenfeld, D. B.
in
639/33/445/846
/ 639/33/525/869
/ 639/766/1960
/ Astrophysics
/ Atomic
/ Aérospatiale, astronomie & astrophysique
/ Cassini mission
/ Classical and Continuum Physics
/ Complex Systems
/ Condensed Matter Physics
/ Current sheets
/ Diffusion
/ Jupiter
/ Jupiter (planet)
/ Kinetics
/ letter
/ Magnetic fields
/ Magnetism
/ Magnetospheres
/ Magnetotails
/ Mathematical and Computational Physics
/ Molecular
/ Optical and Plasma Physics
/ Physical, chemical, mathematical & earth Sciences
/ Physics
/ Physique, chimie, mathématiques & sciences de la terre
/ Planetary magnetospheres
/ Plasma
/ Plasma loss
/ Plasmas
/ Reconfiguration
/ Rotating bodies
/ Rotation
/ Saturn
/ Saturn (planet)
/ Solar system
/ Space science, astronomy & astrophysics
/ Spacecraft
/ Theoretical
/ Wave energy
2016
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Cassini in situ observations of long-duration magnetic reconnection in Saturn’s magnetotail
by
André, N.
, Kidder, A.
, Volwerk, M.
, Lamy, L.
, Sergis, N.
, Poh, G.-K.
, Jia, X.
, Coates, A. J.
, Thomsen, M. F.
, Dougherty, M. K.
, Jackman, C. M.
, Slavin, J. A.
, Arridge, C. S.
, Walsh, A. P.
, Eastwood, J. P.
, Zarka, P.
, Radioti, A.
, Reisenfeld, D. B.
in
639/33/445/846
/ 639/33/525/869
/ 639/766/1960
/ Astrophysics
/ Atomic
/ Aérospatiale, astronomie & astrophysique
/ Cassini mission
/ Classical and Continuum Physics
/ Complex Systems
/ Condensed Matter Physics
/ Current sheets
/ Diffusion
/ Jupiter
/ Jupiter (planet)
/ Kinetics
/ letter
/ Magnetic fields
/ Magnetism
/ Magnetospheres
/ Magnetotails
/ Mathematical and Computational Physics
/ Molecular
/ Optical and Plasma Physics
/ Physical, chemical, mathematical & earth Sciences
/ Physics
/ Physique, chimie, mathématiques & sciences de la terre
/ Planetary magnetospheres
/ Plasma
/ Plasma loss
/ Plasmas
/ Reconfiguration
/ Rotating bodies
/ Rotation
/ Saturn
/ Saturn (planet)
/ Solar system
/ Space science, astronomy & astrophysics
/ Spacecraft
/ Theoretical
/ Wave energy
2016
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Cassini in situ observations of long-duration magnetic reconnection in Saturn’s magnetotail
Journal Article
Cassini in situ observations of long-duration magnetic reconnection in Saturn’s magnetotail
2016
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Overview
Cassini’s encounter with Saturn’s magnetotail — the long magnetosphere region stretching into space — has revealed that plasma exits the magnetosphere through long-duration magnetic reconnection, which ejects ten times more mass than estimated.
Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through which stored magnetic energy associated with current sheets is converted into thermal, kinetic and wave energy
1
,
2
,
3
,
4
. Magnetic reconnection is also thought to be a key process involved in shedding internally produced plasma from the giant magnetospheres at Jupiter and Saturn through topological reconfiguration of the magnetic field
5
,
6
. The region where magnetic fields reconnect is known as the diffusion region and in this letter we report on the first encounter of the Cassini spacecraft with a diffusion region in Saturn’s magnetotail. The data also show evidence of magnetic reconnection over a period of 19 h revealing that reconnection can, in fact, act for prolonged intervals in a rapidly rotating magnetosphere. We show that reconnection can be a significant pathway for internal plasma loss at Saturn
6
. This counters the view of reconnection as a transient method of internal plasma loss at Saturn
5
,
7
. These results, although directly relating to the magnetosphere of Saturn, have applications in the understanding of other rapidly rotating magnetospheres, including that of Jupiter and other astrophysical bodies.
Publisher
Nature Publishing Group UK,Nature Publishing Group,Nature Publishing Group [2005-....],Nature
Subject
/ Atomic
/ Aérospatiale, astronomie & astrophysique
/ Classical and Continuum Physics
/ Jupiter
/ Kinetics
/ letter
/ Mathematical and Computational Physics
/ Physical, chemical, mathematical & earth Sciences
/ Physics
/ Physique, chimie, mathématiques & sciences de la terre
/ Plasma
/ Plasmas
/ Rotation
/ Saturn
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