| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1781462 | Planetary and Space Science | 2012 | 15 Pages |
Abstract
⺠H2O2 is a key trace species of Mars, probably responsible for oxidizing its surface. ⺠We have mapped H2O2 over the seasons using the TEXES imaging spectrometer at IRTF. ⺠The observations favor GCM simulations including heterogeneous chemistry. ⺠Transient H2O2 souces might locally be formed in dust devils/storms. ⺠Present results are reviewed and the detectability of local sources is discussed.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
T. Encrenaz, T.K. Greathouse, F. Lefèvre, S.K. Atreya,