Open AccessSimulation of spontaneous and variable global dust storms with the GFDL Mars GCM
Author(s) -
Basu Shabari,
Wilson John,
Richardson Mark,
Ingersoll Andrew
Publication year - 2006
Publication title -
journal of geophysical research: planets
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2005je002660
Subject(s) - storm , climatology , environmental science , atmospheric sciences , hadley cell , forcing (mathematics) , atmospheric circulation , northern hemisphere , convective storm detection , storm track , geology , general circulation model , climate change , oceanography
We report on the successful simulation of global dust storms in a general circulation model. The simulated storms develop spontaneously in multiyear simulations and exhibit significant interannual variability. The simulated storms produce dramatic increases in atmospheric dustiness, global‐mean air temperatures, and atmospheric circulation intensity, in accord with observations. As with observed global storms, spontaneous initiation of storms in the model occurs in southern spring and summer, and there is significant interannual variability in storm development: years with no storms are interspersed with years with storms of various sizes and specific seasonal date of initiation. Our results support the idea that variable and spontaneous global dust storm behavior can emerge from a periodically forced system (the only forcing being the diurnal and seasonal cycles) when the dust injection mechanism involves an activation threshold. In our simulations, surface wind stresses associated with resolved, large‐scale (>300 km) wind systems initiate the storms. These winds are generally associated with the seasonally migrating CO 2 cap boundary and sloping topography of the Hellas basin, thermal tides, and traveling waves. A very limited number of large storms begin with lifting along the frontal zones associated with traveling waves in the northern hemisphere. Explosive growth to global scales results from the intensification of the Hadley circulation and the activation of secondary dust‐lifting centers.