A review of Martian impact crater ejecta structures and their implications for target properties

By N. Barlow. 2005

149 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/862ea29e3bcf151ca0ae0ff4551b5fea921cd2f6

How researchers see this paper

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

In Aerospace Engineering

1. Nicolas Mangold
2. A. S. McEwen
3. S. Byrne
4. E. Kite

In Astronomy and Astrophysics

1. A. S. McEwen
2. Nicolas Gonzalez Thomas
3. Hirise Team
4. Nicolas Mangold
5. S. Conway
6. B. Langlais
7. V. Ansan
8. S. Adeli

Citations in the corpus

• A chronology of early Mars climatic evolution from impact crater degradation (2012, background): “This map shows that these ejecta extend about two to three crater radii (2R to 3R) from the crater center, typical for this size of crater [e.g., Barlow, 2005].”
• Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) (2007, background): “…cratering has played a large role in sculpting the surface [Strom et al., 1992], but it is unclear whether subtle differences in pristine morphology may reflect the influence of the atmosphere and/or subsurface volatiles during formation [Schultz and Gault, 1979; Schultz, 1992; Barlow, 2005].”