Observations of the initiation and evolution of the 2001 Mars global dust storm
By Melissa J. Strausberg, Huiqun Wang, Mark Richardson, S. Ewald, A. Toigo. 2005
148 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/cac4dafea1e34b9a568acae509e3b24a90453fb1
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In Astronomy and Astrophysics
- Ashwin R. Vasavada
- Á. Vicente-Retortillo
- S. Guzewich
- Michael D. Smith
- M. Bourke
- Michael J. Wolff
- Philip R. Christensen
- J. Bandfield
Citations in the corpus
- Mars Science Laboratory Observations of the 2018/Mars Year 34 Global Dust Storm (2018, background): “…1979; Newman et al., 2002; Wilson, 1997; Zurek, 1982), change surface albedo patterns (e.g., Cantor, 2007; Szwast et al., 2006; Vincendon et al., 2015), and modify subsequent transport and deposition of water and CO 2 at the poles (Benson & James, 2005; Cantor, 2007; Strausberg et al., 2005).”
- Mars Global Digital Dune Database and initial science results (2007, background): “It is possible that dust storms originating in Hellas Planitia [e.g., Strausberg et al., 2005], or other flows related to the topography of Hellas, create easterly winds that are strong and persistent enough to dominate dune morphology.”