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PARTICLE ACCELERATION IN A MODEL OF A TURBULENT RECONNECTING PLASMA: A FRACTIONAL DIFFUSION APPROACH

Bian, N H; Browning, P K

Astrophysical Journal Letters. 2008;687(2):L111-L114.

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Abstract

High-energy charged particles are produced during solar flares. These may be accelerated by the strong electric fields associated with the magnetic reconnection process which is the source of energy release in flares. A simple model of random acceleration of charged particles due to fragmented electric fields is considered for the case of a turbulent reconnecting plasma in which the fluctuating electric field is highly localized and its magnitude distributed according to power laws. The statistical properties of the acceleration process are expressed in terms of a fractional diffusion equation in velocity space, whose solution displays a power-law tail related only to the statistics of the electric field.

Bibliographic metadata

Type of resource:
Content type:
Published date:
Volume:
687
Issue:
2
Start page:
L111
End page:
L114
Digital Object Identifier:
10.1086/593145
ISI Accession Number:
WOS:000262732300015
Related website(s):
  • Related website <Go to ISI>://WOS:000262732300015
General notes:
  • Bian, N. H. Browning, P. K.
Access state:
Active

Institutional metadata

University researcher(s):

Record metadata

Manchester eScholar ID:
uk-ac-man-scw:144194
Created by:
Browning, Philippa
Created:
4th January, 2012, 11:58:42
Last modified by:
Browning, Philippa
Last modified:
4th January, 2012, 11:58:42

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