A One-dimensional Magnetohydrodynamic Model of Solar Flares: Emergence of a Population of Weak Events, and a Possible Road toward Nanoflares

Details A One-dimensional Magnetohydrodynamic Model of Solar Flares: Emergence of a Population of Weak Events, and a Possible Road toward Nanoflares A One-dimensional Magnetohydrodynamic Model of Solar Flares: Emergence of a Population of Weak Events, and a Possible Road toward Nanoflares

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...521..483g&link_type=abstract

The Astrophysical Journal, Volume 521, Issue 1, pp. 483-489.

Astronomy and Astrophysics

Astronomy

11

Magnetohydrodynamics: Mhd, Sun: Corona, Sun: Flares, Turbulence

Scientific paper

Impulsive dynamical processes in the solar corona, such as the flaring of magnetic loops, can be modeled by compressible one-dimensional magnetohydrodynamic (MHD) equations with a forcing that mimics the erratic motion of the magnetic footpoints. Two different kinds of dissipative events are observed in such a model, the study of which sustains the image of an efficient heating by a swarm of small events.

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