![](/images/icons/spacer.gif) |
Detailed Reference Information |
Ryan, J.A., Sharman, R.D. and Lucich, R.D. (1981). Local Mars dust storm generation mechanism. Geophysical Research Letters 8: doi: 10.1029/GL008i008p00899. issn: 0094-8276. |
|
On Ls = 340¿, first Mars year of Viking on the surface, a local dust storm was observed at the Viking Lander no.1 site by Viking Orbiter A. The storm lasted less than one martian day (sol) with the dust raised affecting the site for about three sols. It is concluded that this storm was caused by baroclinic waves and that the threshold wind speed for saltation was 25--30 m sec-1. |
|
![](/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) |
|
|
|
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) |