Aerosol vertical profile on Mars from the measurements of thermal radiation on the limb

Moroz, V.I.; Gektin, Yu. M.; Naraeva, M. K.; Selivanov, A. S.; Титов, Д. В.

doi:10.1016/0032-0633(94)90064-7

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Cloud Particle Characteristics1

Introduction1

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1994

2024

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Cited by 14 publications

(2 citation statements)

References 27 publications

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“…with condensation on the local level and with approximately uniform mixing from below. This is in agreement The typical cloud layer should contain (0.7-1.5) ϫ with studies by Davies (1979), who derived a constant of the altitude determination makes extrapolation below 10-15 km less accurate. Extrapolation down to the 6-mbar mixing ratio of 160 ppmv in the lowest scale height, and Clancy et al (1992), 100 ppmv.…”

Section: Cloud Particle Characteristicssupporting

confidence: 78%

Vertical Distribution of Water in the Near-Equatorial Troposphere of Mars: Water Vapor and Clouds

Rodin¹,

Korablev²,

Мороз³

1997

Icarus

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Section: Cloud Particle Characteristicssupporting

confidence: 78%

Vertical Distribution of Water in the Near-Equatorial Troposphere of Mars: Water Vapor and Clouds

Rodin¹,

Korablev²,

Мороз³

1997

Icarus

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“…The dust is vertically distributed with a scale height, H, of 11.3 km, equal to the gas scale height at initial conditions: a constant mixing ratio. This is consistent with the results from the Phobos mission [ Moroz et al , 1993].…”

Section: Introductionmentioning

confidence: 99%

A model of dust in the Martian lower atmosphere

Davy¹,

Taylor²,

Weng³

et al. 2009

J. Geophys. Res.

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[1] A coupled boundary layer-Aeolian dust model of the Martian atmosphere is presented. This model was developed to determine how radiation (scattering, absorption, and emission) by dust affects the boundary layer and, in turn, how this affects the dust distribution in the atmosphere. This was achieved by coupling a planetary boundary layer (PBL) model with the 2007 dust model of P. A. Taylor et al. The principle motivation here is to determine whether it will be possible to use the lidar on board the Phoenix lander to detect the depth of the Martian boundary layer from the dust distribution. Runs were conducted for different dust profiles, roughness lengths, and geostrophic winds. These indicate that there should be a distinct horizon in dust concentration which will be detectable by the Phoenix lidar. The model is also applied to the 1977B dust storm optical data of Viking Lander 1, and our analysis indicates a significant improvement over previous 1-D studies of dust storm decay.

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Observations of water vapour anomaly above Tharsis volcanoes on Mars in the ISM (Phobos-2) experiment

Titov

Мороз

Grigoriev

et al. 1994

Planetary and Space Science

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Aerosol vertical profile on Mars from the measurements of thermal radiation on the limb

Cited by 14 publications

References 27 publications

Vertical Distribution of Water in the Near-Equatorial Troposphere of Mars: Water Vapor and Clouds

Vertical Distribution of Water in the Near-Equatorial Troposphere of Mars: Water Vapor and Clouds

A model of dust in the Martian lower atmosphere

Observations of water vapour anomaly above Tharsis volcanoes on Mars in the ISM (Phobos-2) experiment

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