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MARCI-Observed Clouds in the Hellas Basin during Northern Hemisphere Summer on Mars: Interpretation with the NASA/Ames Legacy Mars Global Climate ModelWe present a study that is motivated by a population of water ice clouds in the Hellas Basin that has been observed by the MARs Color Imager (MARCI) instrument on the Mars Reconnaissance Orbiter (MRO) to persist throughout the majority of Northern Hemisphere (NH) summer. Although water ice clouds are present in Hellas at very low opacities throughout NH spring, they noticeably thicken after L(sub s) 60° and continue to do so until their peak optical thickness is attained at L(sub s) ~120°. They dissipate rapidly from L(sub s) 120° to 150°, and by L(sub s) 150°, the only clouds in Hellas are on the southern side of the basin and are indistinguishable from the polar hood clouds. We use the NASA/Ames Legacy Mars Global Climate Model (GCM), which is supported by the Agency’s Mars Climate Modeling Center, to investigate the dynamical and microphysical mechanisms that control the formation and evolution of Hellas water ice clouds. We show that water is transported from the North Polar Residual Cap (NPRC) southward across the equator and into the Hellas region. Water vapor is confined down low by cloud formation in the aphelion cloud belt, thus limiting the effectiveness of transport by the zonal mean overturning circulation (i.e., the Hadley cell). Thus, contrary to the commonly held conceptual understanding that the Hadley cell controls cross-equatorial water transport during this season, we show that the southward transport of water is done primarily in the vapor phase by stationary eddies at nearly all latitudes, including across the equator. Clouds form near the surface in the basin as moist air mixes with cold polar air on the western side of Hellas and are subsequently transported clockwise around the north side of the basin by the low-level cyclonic circulation. The simulated Hellas clouds have small particle sizes (~3–5 μm), are very low, and exist as long as the NPRC is exposed.
Document ID
20200002856
Acquisition Source
Ames Research Center
Document Type
Reprint (Version printed in journal)
Authors
M. A. Kahre
(Ames Research Center Mountain View, California, United States)
R. M. Haberle
(Ames Research Center Mountain View, California, United States)
J. L. Hollingsworth
(Ames Research Center Mountain View, California, United States)
M. J. Wolff ORCID
(Space Science Institute Boulder, Colorado, United States)
Date Acquired
April 21, 2020
Publication Date
October 28, 2019
Publication Information
Publication: Icarus
Publisher: Elsevier
Volume: 338
Issue Publication Date: March 1, 2020
ISSN: 0019-1035
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN79187
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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