Image Details
Caption: Fig. 7.
Evolution of shock velocity for a shock moving with mean velocity 150 km s−1. We show the effect of short‐wavelength upstream density perturbations by comparing the cases of (top) no, (middle) small‐, and (bottom) large‐amplitude fluctuations. The line segment in the bottom panel indicates an interval 10 times the fluctuation timescale τ.
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.