Heating plasma loops in the solar corona

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Ashbourn, J. M. A. and Woods, L. C. and Bingham, R. (2001) Heating plasma loops in the solar corona. Astrophysical Journal, 553 (2). pp. 941-948. ISSN 1538-4357 (https://doi.org/10.1086/320956)

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Abstract

We find a new heat source term for hot coronal loops and include it in the energy equation. This term requires the loop to be hotter than the ambient corona and depends on the combined effect of electron fluid shear and the temperature gradient. Under certain circumstances, the shear drives the heat up the radial temperature gradient into a cross section of the magnetic flux tube from which it leaves by radiation and by conduction down the axial temperature gradient in the usual manner. The heat source is thus a surface term applied over the whole of the loop rather than a volume-distributed term, and its strength is proportional to the cube of the temperature. We apply it to the usual scaling law and obtain an expression for the radius of the flux tube for thermal equilibrium to hold. The temperature distribution around the plasma loop is determined and compared with recent observations and is found to be in satisfactory agreement with them.

ORCID iDs

Ashbourn, J. M. A., Woods, L. C. and Bingham, R. ORCID logoORCID: https://orcid.org/0000-0002-9843-7635;
  • Item type:Article
    ID code:51970
    Dates:
    Date
    Event
    1 June 2001
    Published
    7 February 2001
    Accepted
    Notes:(c) American Astronomical Society
    Subjects:Science > Physics
    Department:Faculty of Science > Physics
    Depositing user: Pure Administrator
    Date deposited:26 Feb 2015 15:18
    Last modified:11 Nov 2024 10:59
    Related URLs:
    URI:https://strathprints.strath.ac.uk/id/eprint/51970
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