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The Hydrodynamic Evolution of Impulsively Heated Coronal Loops: Explicit Analytical Approximations

  • Authors: Markus J. Aschwanden and David Tsiklauri

ASCHWANDEN & TSIKLAURI 2009 The Astrophysical Journal Supplement Series 185 171.

  • Provider: AAS Journals

Caption: Figure 4.

Heating rate E H ( t) is given by a Gaussian function (thin solid curve). The density function n( t) follows the time integral (thick solid curve) of this Gaussian function (for a constant value of dn evap/ dE H ) according to the Neupert effect, which can be approximated by a semi-Gaussian function (dashed curve). The time t m of the maximum heating rate and the time t p of the peak density are indicated with dotted lines.

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