The case for quasi-steady models in describing the physics of dayside merging
Article first published online: 3 JUN 2011
©1996. American Geophysical Union. All Rights Reserved.
Eos, Transactions American Geophysical Union
Volume 77, Issue 26, page 246, 25 June 1996
How to Cite
1996), The case for quasi-steady models in describing the physics of dayside merging, Eos Trans. AGU, 77(26), 246–246, doi:10.1029/96EO00176., and (
- Issue published online: 3 JUN 2011
- Article first published online: 3 JUN 2011
- Cited By
The magnetosphere varies on all measured temporal and spatial scales. Because this variability is apparent in so many data sets, and because dynamical behavior is intrinsically exciting, a large majority of space physicists have always emphasized transients. We quite agree that merging transients exist, although we believe that they are directly driven by the variable input from the magnetosheath (we have proposed examples ourselves). In emphasizing “quasi-steady” in this discussion, we only mean that specifying the interplanetary magnetic field (IMF) and solar wind conditions (or more precisely, magnetosheath conditions) also pretty well specifies the state of the dayside magnetosphere.