TY - JOUR
T1 - Martian dust devil statistics from high-resolution large-eddy simulations
AU - Nishizawa, Seiya
AU - Odaka, Masatsugu
AU - Takahashi, Yoshiyuki O.
AU - Sugiyama, Ko Ichiro
AU - Nakajima, Kensuke
AU - Ishiwatari, Masaki
AU - Takehiro, Shin Ichi
AU - Yashiro, Hisashi
AU - Sato, Yousuke
AU - Tomita, Hirofumi
AU - Hayashi, Yoshi Yuki
N1 - Publisher Copyright:
© 2016. American Geophysical Union. All Rights Reserved.
PY - 2016/5/16
Y1 - 2016/5/16
N2 - Dust devils are one of the key elements in the Martian atmospheric circulation. In order to examine their statistics, we conducted high-resolution (up to 5 m) and wide-domain (about 20 × 20 km2) large-eddy simulations of the Martian daytime convective layer. Large numbers of dust devils developed spontaneously in the simulations, which enabled us to represent a quantitative consideration of Martian dust devil frequency distributions. We clarify the distributions of size and intensity, a topic of debate, and conclude that the maximum vertical vorticity of an individual dust devil has an exponential distribution, while the radius and circulation have power law distributions. A grid refinement experiment shows that the rate parameter of the vorticity distribution and the exponent of the circulation distribution are robust. The mode of the size distribution depends on the resolution, and it is suggested that the mode is less than 5 m.
AB - Dust devils are one of the key elements in the Martian atmospheric circulation. In order to examine their statistics, we conducted high-resolution (up to 5 m) and wide-domain (about 20 × 20 km2) large-eddy simulations of the Martian daytime convective layer. Large numbers of dust devils developed spontaneously in the simulations, which enabled us to represent a quantitative consideration of Martian dust devil frequency distributions. We clarify the distributions of size and intensity, a topic of debate, and conclude that the maximum vertical vorticity of an individual dust devil has an exponential distribution, while the radius and circulation have power law distributions. A grid refinement experiment shows that the rate parameter of the vorticity distribution and the exponent of the circulation distribution are robust. The mode of the size distribution depends on the resolution, and it is suggested that the mode is less than 5 m.
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U2 - 10.1002/2016GL068896
DO - 10.1002/2016GL068896
M3 - Article
AN - SCOPUS:84969922347
SN - 0094-8276
VL - 43
SP - 4180
EP - 4188
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 9
ER -