Figure 9 from Turbulence and Magnetic Field Amplification in Supernova Remnants: Interactions Between a Strong Shock Wave and Multiphase Interstellar Medium

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Turbulence and Magnetic Field Amplification in Supernova Remnants: Interactions Between a Strong Shock Wave and Multiphase Interstellar Medium

Authors: Tsuyoshi Inoue, Ryo Yamazaki, and Shu-ichiro Inutsuka

INOUE, YAMAZAKI, & INUTSUKA 2009 The Astrophysical Journal 695 825.

Provider: AAS Journals

Caption: Figure 9.

Evolutions of the maximum (thick lines) and average (thin lines) field strengths (top), and the local plasma βs at the point where the magnetic field strength is maximum (bottom). The red, green, blue, and black lines are the results of Models 1, 2, 3, and 4, respectively.

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