**Theory of magnetic reconnection in solar and astrophysical plasmas.** / Pontin, D.I.

Research output: Contribution to journal › Article

Pontin, DI 2012, 'Theory of magnetic reconnection in solar and astrophysical plasmas' *Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences*, vol 370, no. 1970, pp. 3169-3192., 10.1098/rsta.2011.0501

Pontin, D. I. (2012). Theory of magnetic reconnection in solar and astrophysical plasmas. *Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences*, *370*(1970), 3169-3192. 10.1098/rsta.2011.0501

Pontin DI. Theory of magnetic reconnection in solar and astrophysical plasmas. Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences. 2012 Jul 13;370(1970):3169-3192. Available from: 10.1098/rsta.2011.0501

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title = "Theory of magnetic reconnection in solar and astrophysical plasmas",

author = "D.I. Pontin",

note = "Copyright 2012 Elsevier B.V., All rights reserved.",

year = "2012",

month = "7",

doi = "10.1098/rsta.2011.0501",

volume = "370",

pages = "3169--3192",

journal = "Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences",

issn = "1364-503X",

number = "1970",

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TY - JOUR

T1 - Theory of magnetic reconnection in solar and astrophysical plasmas

AU - Pontin,D.I.

N1 - Copyright 2012 Elsevier B.V., All rights reserved.

PY - 2012/7/13

Y1 - 2012/7/13

N2 - Magnetic reconnection is a fundamental process in a plasma that facilitates the release of energy stored in the magnetic field by permitting a change in the magnetic topology. In this paper, we present a review of the current state of understanding of magnetic reconnection. We discuss theoretical results regarding the formation of current sheets in complex three-dimensional magnetic fields and describe the fundamental differences between reconnection in two and three dimensions. We go on to outline recent developments in modelling of reconnection with kinetic theory, as well as in the magnetohydrodynamic framework where a number of new three-dimensional reconnection regimes have been identified. We discuss evidence from observations and simulations of Solar System plasmas that support this theory and summarize some prominent locations in which this new reconnection theory is relevant in astrophysical plasmas. This journal is © 2012 The Royal Society.

AB - Magnetic reconnection is a fundamental process in a plasma that facilitates the release of energy stored in the magnetic field by permitting a change in the magnetic topology. In this paper, we present a review of the current state of understanding of magnetic reconnection. We discuss theoretical results regarding the formation of current sheets in complex three-dimensional magnetic fields and describe the fundamental differences between reconnection in two and three dimensions. We go on to outline recent developments in modelling of reconnection with kinetic theory, as well as in the magnetohydrodynamic framework where a number of new three-dimensional reconnection regimes have been identified. We discuss evidence from observations and simulations of Solar System plasmas that support this theory and summarize some prominent locations in which this new reconnection theory is relevant in astrophysical plasmas. This journal is © 2012 The Royal Society.

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U2 - 10.1098/rsta.2011.0501

DO - 10.1098/rsta.2011.0501

M3 - Article

VL - 370

SP - 3169

EP - 3192

JO - Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences

T2 - Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences

JF - Philosophical Transactions of the Royal Society A - Mathematical Physical and Engineering Sciences

SN - 1364-503X

IS - 1970

ER -