Figure 10 from The Hydrodynamic Evolution of Impulsively Heated Coronal Loops: Explicit Analytical Approximations

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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 10.

Temperature (left) and density profiles (right) for a subset of cases simulated in Tsiklauri et al. (2004) with varying loop lengths, from L = 13.8 Mm (top) to L = 110 Mm (bottom). Major discrepancies are only found for the shortest loops (top).

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