Modeling the Martian dust cycle, 1. Representations of dust transport processes

By C. E. Newman, S. R. Lewis, Peter L Read, Francois Forget. 2002

270 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Earth-Surface Processes

View Paper: https://www.semanticscholar.org/paper/77b14a11ea264b1ec8d9d55c7518a1d9ed96add7

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Citations in the corpus

The Modern Near-Surface Martian Climate: A Review of In-situ Meteorological Data from Viking to Curiosity (2017, background): “The large spatial and temporal variability in atmospheric dust content creates complex feedbacks connecting dust lifting and transport with the evolving atmospheric circulations (Newman et al. 2002a, 2002b; Basu et al. 2004; Kahre et al. 2006; Madeleine et al. 2011).”
Mars Science Laboratory Observations of the 2018/Mars Year 34 Global Dust Storm (2018, methodology): “They radically alter atmospheric circulation (Conrath, 1975; Guzewich et al., 2014; Haberle et al., 1982; Leovy & Zurek, 1979; Newman et al., 2002; Wilson, 1997; Zurek, 1982), change surface albedo patterns (e.”
THE MARTIAN ATMOSPHERIC BOUNDARY LAYER (2011, methodology): “On Mars, however, lf ∼ 5–10 mm and a much larger fraction of the aerosol spectra effectively moves in a slip flow [cf. Newman et al., 2002a].”
Incorporating the effect of small‐scale circulations upon dust emission in an atmospheric general circulation model (2004, unknown): “This mechanism of small-scale mixing is similarly believed to be the main process of dust injection into the Martian atmosphere [Newman et al., 2002; Leovy, 2003].”
Revisiting the radiative impact of dust on Mars using the LMD Global Climate Model (2011, methodology): “linear and threshold‐linked behavior [Newman et al., 2002; Basu et al., 2004; Kahre et al., 2008], might be responsible for the rapid increase in the observed temperature during the rise of dust storm events and is not captured by our model in”
Dust devils on Earth and Mars (2006, methodology): “’’ Newman et al. [2002] used two parameterizations, one in which the dust devil injection flux was simply proportional to L and another that”
Simulation of the Martian dust cycle with the GFDL Mars GCM (2004, background): “Several small dust storms are generated in the northern early autumn and later winter, associated with low-pressure frontal storms, as described by Wang et al. [2003], and also generated in the Oxford Mars GCM [Newman et al., 2002b].”
A new model to simulate the Martian mesoscale and microscale atmospheric circulation: Validation and first results (2009, background): “…et al. , 2005], on the slope irradiance estimations [ Spiga and Forget , 2008], on the dust lifting and sedimentation [ Forget et al. , 1999b; Newman et al. , 2002], on the water cycle and water ice clouds [ Montmessin et al. , 2004], and on the photochemical species [ Lefe`vre et al. ,…”