Standardizing the nomenclature of Martian impact crater ejecta morphologies

By N. G. Barlow, J. M. Boyce, F. Costard, R. Craddock, J. B. Garvin, H. Susane, Sakimoto, R. Kuzmin, D. Roddy, L. Soderblom. 2000

196 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/aaeb733ff8d272144eb5fd1c69502284e8fa1dfe

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In Aerospace Engineering

1. James F. Bell III
2. R. Clancy
3. Michael A. Caplinger
4. Michael C. Malin
5. M. Ravine
6. B. Cantor
7. R. Haberle
8. Michael J. Wolff

In Astronomy and Astrophysics

1. Michael D. Smith
2. Michael J. Wolff
3. B. Cantor
4. R. Haberle
5. James F. Bell III
6. R. Clancy
7. K. Edgett
8. Michael C. Malin

Citations in the corpus

• Context Camera Investigation on board the Mars Reconnaissance Orbiter (2007, background): “[49] On Mars, some craters exhibit ‘‘flow’’ or ‘‘rampart’’ ejecta (now termed ‘‘layered’’ according to a consortium of investigators [Barlow et al., 2000]), believed by many to reflect the influence of subsurface volatiles on ejecta distri-”
• Mars Global Surveyor Mars Orbiter Camera: Interplanetary cruise through primary mission (2001, background): “…beneath a large "pedestal" crater (craters whose ejecta appears raised above the surrounding terrain by eolian deflation of that terrain, where crater ejecta has served as an armor to protect underlying material from erosion [McCauley, 1973], Barlow et al. 2000) in Arabia Terra (Figure 29).”