| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701590 | Icarus | 2013 | 8 Pages |
Abstract
⺠Atmospheric pressure affects the distribution of pyroclasts on Mars. ⺠Higher atmospheric pressure causes pyroclasts to be deposited in narrower bands. ⺠Pyroclasts dispersal under all pressure regimes is dominated by zonal winds. ⺠Pyroclasts will be dominantly deposited to the east or west of an edifice.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Laura Kerber, François Forget, Jean-Baptiste Madeleine, Robin Wordsworth, James W. Head, Lionel Wilson,