Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 18 January 1980:
Vol. 207. no. 4428, pp. 301 - 302
DOI: 10.1126/science.207.4428.301

Articles

Corotation Lag in Jupiter's Magnetosphere: Comparison of Observation and Theory

T. W. HILL 1

1 Department of Space Physics and Astronomy, Rice University, Houston, Texas 77001

Voyager 1 plasma flow data are compared with a recent theory that predicted measurable departures from rigid corotation in Jupiter's magnetosphere as a consequence of rapid plasma production and weak atmosphere-magnetosphere coupling. The comparison indicates that the theory can account for the observed corotation lag, provided that the plasma mass production rate during the Voyager 1 encounter was rather larger than expected, namely sim 1030 atomic mass units per second.

Submitted on August 28, 1979





To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)