Simulation of the Martian dust cycle with the GFDL Mars GCM

By S. Basu, Mark Richardson, Robert J. Wilson. 2004

181 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/336e1c3a7a21024b8f0efaa5dbe995d329396025

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In Astronomy and Astrophysics

Citations in the corpus

The physics of wind-blown sand and dust (2012, background): “Aeolian versus underwater bedforms. Experiments of dune formation under water provide a means to study the longterm dynamics of sand dunes (see section 3.1.6.5). Much effort has been dedicated to understanding the different mechanisms of transport and bedform dynamics under water (Fourrière et al 20”
Convective vortices and dust devils at the Phoenix Mars mission landing site (2010, background): “, 2003] and influence the global dust cycle on Mars by maintaining the background dust load in the atmosphere [Ryan and Lucich, 1983; Basu et al., 2004; Cantor et al., 2006].”
Observations of the initiation and evolution of the 2001 Mars global dust storm (2005, methodology): “An initial GCM study of dust storm evolution resulting from a source in Hellas, but at a somewhat later season, shows transport in both eastward and westward directions, which is contrary to observations [Basu et al., 2004].”
Revisiting the radiative impact of dust on Mars using the LMD Global Climate Model (2011, methodology): “Elevated dust layers are also shown by Basu et al. [2006], andWilson et al.”
Dust devils on Earth and Mars (2006, methodology): “Newman et al. [2002] tuned their scheme to match observations of opacity and presented their results in arbitrary units of flux, whereas Basu et al. [2004] tuned their free parameter to match year-round air temperature and used the ‘‘best fit’’ value to determine L. [67] Newman et al. [2002] found”
Modeling the Martian dust cycle and surface dust reservoirs with the NASA Ames general circulation model (2006, methodology): “Additionally, little discussion of the nature of the simulated interannual variability is presented by Basu et al. [2004] , making direct comparisons between their results and ours difficult.”
The Modern Near-Surface Martian Climate: A Review of In-situ Meteorological Data from Viking to Curiosity (2017, background): “…Martian atmosphere transports large amounts of dust, which interacts with solar and infrared radiation, regulating atmospheric and surface heating rates and thus influencing the Martian climate (Gierasch and Goody 1972; Kahn et al. 1992; Forget et al. 1999; Basu et al. 2004; Madeleine et al. 2011).”
A new model to simulate the Martian mesoscale and microscale atmospheric circulation: Validation and first results (2009, background): “…, bu t on l y i nd i ca t e s t h e m a x i m a l v a l u e o f ho r i z on t a l r e s o l u ti on f o r t h e l a tit ud oo r d i n a t e s ( po l e w a r ec r ea s e du e t o t h e M e r ca t o r p r o j ec ti on ) . rate [ Basu et al. , 2004] leads us to postpone these issues to future studies.”
Constraints on dust aerosols from the Mars Exploration Rovers using MGS overflights and Mini‐TES (2006, background): “Figure 25 shows an example from the Mars GCM of R. J. Wilson et al. (personal communication, 2006) [see also Hinson and Wilson, 2004; Basu et al., 2004 ].”