Assimilating and Modeling Dust Transport in the Martian Climate System

Ruan, Tao; Montabone, Luca; Read, Peter L. and Lewis, Stephen R. (2012). Assimilating and Modeling Dust Transport in the Martian Climate System. In: IAU Symposium 293: Formation, Detection, and Characterization of Extrasolar Habitable Planets, 20-31 Aug 2012, Beijing, China.

DOI: https://doi.org/10.1017/s1743921313013094

Abstract

A meteorological data assimilation system has been developed recently for analyzing measurements of temperature and dust opacity on Mars and has been successfully applied in several studies (e.g. Montabone et al. 2005, Lewis et al. 2007) to study various atmospheric phenomena. A more sophisticated data assimilation system, now with full dust transport incorporated, is becoming available to represent more accurately and realistically the physical transport of dust.

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• Item ORO ID
• 35438
• Item Type
• Conference or Workshop Item
• Extra Information
• Formation, Detection, and Characterization of Extrasolar Habitable Planets, Proceedings IAU Symposium No. 293, 2012
• Keywords
• hydrodynamics, planets and satellites: general, methods: data analysis, methods: numerical
• Academic Unit or School
• Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
  Faculty of Science, Technology, Engineering and Mathematics (STEM)
• Research Group
• Space
• Copyright Holders
• © 2012 International Astronomical Union
• Related URLs
• • http://www.ifa.hawaii.edu/iau293/(Other)
• Depositing User
• Stephen Lewis