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Self-Similar Evolution of Cosmic Ray Modified Shocks

Self-Similar Evolution of Cosmic Ray Modified Shocks. Hyesung Kang Pusan National University, KOREA. Thermal E. CR E. - kinetic energy flux through shocks F k = (1/2) r 1 V s 3. - net thermal energy flux generated at shocks F th = (3/2) [P 2 -P 1 (r 2 /r 1 ) g ] u 2

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Bohm type diffusion - PowerPoint PPT Presentation

Self-Similar Evolution of Cosmic Ray Modified Shocks