Convective vortices and dust devils at the Phoenix Mars mission landing site

By M. D. Ellehoj, H. P. Gunnlaugsson, P. Taylor, Henrik Kahanpää, K. Bean, B. Cantor, B. T. Gheynani, L. Drube, D. Fisher, A. Harri and 9 more. 2010

149 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Physiology

View Paper: https://www.semanticscholar.org/paper/8244396852d2133ffb07b23ce7b816d8c6f4551b

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. Mark T. Lemmon
5. Mark Richardson
6. B. Cantor
7. James F. Bell III
8. Peter H. Smith

In Physiology

1. Michael D. Smith
2. Ashwin R. Vasavada
3. B. Cantor
4. Germán Martínez
5. Nilton O. Renno

Citations in the corpus

• Dust aerosol, clouds, and the atmospheric optical depth record over 5 Mars years of the Mars Exploration Rover mission (2014, background): “operated through November 2006. For that time, MOC provided nearly continuous daily global mapping of the Martian surface at 7.5 km pixel-1 in two band passes, red (600-650 nm) and blue (400-450 nm) [Malin et al. 2010]. In the spirit of mutual collaboration between missions, MOC and later the Mars R”
• The Modern Near-Surface Martian Climate: A Review of In-situ Meteorological Data from Viking to Curiosity (2017, background): “On time-scales ranging from a few seconds to minutes, convective dust devils also induce measurable changes in surface pressure (Ellehoj et al. 2010; Kahanpää et al. 2016; Steakley and Murphy 2016).”