Local Mars dust storm generation mechanism

J. A. Ryan; R. D. Sharman; R. D. Lucich

doi:10.1029/GL008i008p00899

Local Mars dust storm generation mechanism

J. A. Ryan
, R. D. Sharman
, R. D. Lucich

Research output: Contribution to journal › Article › peer-review

15 Scopus citations

Abstract

On L_s = 340°, first Mars year of Viking on the surface, a local dust storm was observed at the Viking Lander #1 site by Viking Orbiter A. The storm lasted less than one martian day (sol) with the dust raised affecting the site for about three sols. It is concluded that this storm was caused by baroclinic waves and that the threshold wind speed for saltation was 25‐30 m sec⁻¹.

Original language	English
Pages (from-to)	899-901
Number of pages	3
Journal	Geophysical Research Letters
Volume	8
Issue number	8
DOIs	https://doi.org/10.1029/GL008i008p00899
State	Published - Aug 1981

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title = "Local Mars dust storm generation mechanism",

abstract = "On Ls = 340°, first Mars year of Viking on the surface, a local dust storm was observed at the Viking Lander \#1 site by Viking Orbiter A. The storm lasted less than one martian day (sol) with the dust raised affecting the site for about three sols. It is concluded that this storm was caused by baroclinic waves and that the threshold wind speed for saltation was 25‐30 m sec−1.",

author = "Ryan, \{J. A.\} and Sharman, \{R. D.\} and Lucich, \{R. D.\}",

year = "1981",

month = aug,

doi = "10.1029/GL008i008p00899",

language = "English",

volume = "8",

pages = "899--901",

journal = "Geophysical Research Letters",

issn = "0094-8276",

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T1 - Local Mars dust storm generation mechanism

AU - Ryan, J. A.

AU - Sharman, R. D.

AU - Lucich, R. D.

PY - 1981/8

Y1 - 1981/8

N2 - On Ls = 340°, first Mars year of Viking on the surface, a local dust storm was observed at the Viking Lander #1 site by Viking Orbiter A. The storm lasted less than one martian day (sol) with the dust raised affecting the site for about three sols. It is concluded that this storm was caused by baroclinic waves and that the threshold wind speed for saltation was 25‐30 m sec−1.

AB - On Ls = 340°, first Mars year of Viking on the surface, a local dust storm was observed at the Viking Lander #1 site by Viking Orbiter A. The storm lasted less than one martian day (sol) with the dust raised affecting the site for about three sols. It is concluded that this storm was caused by baroclinic waves and that the threshold wind speed for saltation was 25‐30 m sec−1.

UR - https://www.scopus.com/pages/publications/0001296527

U2 - 10.1029/GL008i008p00899

DO - 10.1029/GL008i008p00899

M3 - Article

AN - SCOPUS:0001296527

SN - 0094-8276

VL - 8

SP - 899

EP - 901

JO - Geophysical Research Letters

JF - Geophysical Research Letters

IS - 8

ER -

Local Mars dust storm generation mechanism

Abstract

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