![](/images/icons/spacer.gif) |
Detailed Reference Information |
Hunten, D.M., Hoffmann, W.F. and Sprague, A.L. (1994). Jovian seismic waves and their detection. Geophysical Research Letters 21: doi: 10.1029/94GL01060. issn: 0094-8276. |
|
The impacts of the pieces of Comet Shoemaker--Levy 9 should generate strong waves and fronts. Those that start out downward within a few degrees of vertical can travel large distances before reaching the surface again, and may probe to depths (13000 km) as great as the metallic-hydrogen boundary. It is shown that the wave fronts should be detectable through their stratospheric heating and cooling, by imaging in the 7.8 &mgr;m band of CH4, which is very temperature sensitive (radiance ∝T12.3). In addition to the ''seismic'' waves, the experiment should be able to detect slower-moving ducted acoustic waves near the tropopause and still slower gravity waves. ¿ American Geophysical Union 1994 |
|
![](/images/icons/spacer.gif) |
![](/images/icons/spacer.gif) |
BACKGROUND DATA FILES |
|
![](../images/icons/sq.gif) |
Abstract![](/images/icons/spacer.gif) |
|
![](../images/buttons/download.very.flat.gif) |
|
|
|
Keywords
Atmospheric Composition and Structure, Pressure, density, and temperature, Exploration Geophysics, Seismic methods, Planetology, Comets and Small Bodies, Instruments and techniques, Planetology, Fluid Planets, Instruments and techniques |
|
Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
|
|
![](/images/icons/spacer.gif) |