Image Details
Caption: Fig. 4.
Intensity autocorrelation functions for both components of PSR B1937+21 using only left circular polarization. These ACFs were calculated in pulse phase regions that did not include the giant pulses. The time resolution is 0.1 μs. Similar results are obtained using right circular polarization.
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.