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Chromospheric Evaporation via Alfvén Waves

  • Authors: Gerhard Haerendel

HAERENDEL 2009 The Astrophysical Journal 707 903.

  • Provider: AAS Journals

Caption: Figure 7.

Plasma pressure, p, plasma beta, β, external magnetic field, B 0, and corresponding densities for two temperatures ( T i = T e ) of the loop-top plasma as a function of the internal magnetic field, B i , as derived from Equation (6).

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