Observations of martian gullies and constraints on potential formation mechanisms

By J. Heldmann, M. Mellon. 2004

187 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Physiology

View Paper: https://www.semanticscholar.org/paper/705018f72f3ee0b42bc5abcdab67cce9456373bb

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Michael D. Smith
2. Michael J. Wolff
3. R. Haberle
4. B. Cantor
5. James F. Bell III
6. R. Clancy
7. A. S. McEwen
8. M. Ravine

In Physiology

1. B. Cantor
2. C. Dundas
3. A. S. McEwen
4. S. Diniega

Citations in the corpus

• Long-term monitoring of martian gully formation and evolution with MRO/HiRISE (2015, background): “At higher latitudes Heldmann and Mellon (2004) report a transition to equator-facing and then back to pole-facing, while Balme et al. (2006) found little preference.”
• Context Camera Investigation on board the Mars Reconnaissance Orbiter (2007, background): “The channels usually originate at a point about 200–800 m below the local surface outside of the depression in which the gully occurs [Malin and Edgett, 2000b; Gilmore and Phillips, 2002; Heldmann and Mellon, 2004].”