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Mars Science Laboratory Observations of the 2018/Mars Year 34 Global Dust StormMars Science Laboratory Curiosity rover observations of the 2018/Mars year 34 global/planet-encircling dust storm represent the first in situ measurements of a global dust storm with dedicated meteorological sensors since the Viking Landers. The Mars Science Laboratory team planned and executed a science campaign lasting approximately 100 Martian sols to study the storm involving an enhanced cadence of environmental monitoring using the rover's meteorological sensors, cameras, and spectrometers. Mast Camera 880-nanometer optical depth reached 8.5, and Rover Environmental Monitoring Station measurements indicated a 97 percent reduction in incident total ultraviolet solar radiation at the surface, 30 degrees Kelvin reduction in diurnal range of air temperature, and an increase in the semidiurnal pressure tide amplitude to 40 pascals. No active dust-lifting sites were detected within Gale Crater, and global and local atmospheric dynamics were drastically altered during the storm. This work presents an overview of the mission's storm observations and initial results.
Document ID
20190001691
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Guzewich, Scott D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lemmon, M.
(Texas A&M Univ. College Station, TX, United States)
Smith, C. L.
(York University Toronto, Ontario, Canada)
Martinez, G.
(Michigan Univ. Ann Arbor, MI, United States)
de Vicente-Retortillo, A.
(Michigan Univ. Ann Arbor, MI, United States)
Newman, C. E.
(Aeolis Research, Inc. Pasadena, CA, United States)
Baker, M.
(Johns Hopkins Univ. Baltimore, MD, United States)
Campbell, C.
(York University Toronto, Ontario, Canada)
Cooper, B.
(York University Toronto, Ontario, Canada)
Gomez-Elvira, J.
(Centro de Astrobiología (CSIC-INTA) Madrid, Spain)
Harri, A.-M.
(Finnish Meteorological Institute Helsinki, Finland)
Hassler, D.
(Southwest Research Inst. Boulder, CO, United States)
Martin-Torres, F. J.
(Lulea Univ. of Technology Lulea, Sweden)
McConnochie, T.
(Maryland Univ. College Park, MD, United States)
Moores, J. E.
(York University Toronto, Ontario, Canada)
Kahanpaa, H.
(Finnish Meteorological Institute Helsinki, Finland)
Khayat, A.
(Maryland Univ. College Park, MD, United States)
Richardson, M. I.
(Aeolis Research, Inc. Pasadena, CA, United States)
Smith, M. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Sullivan, R.
(Cornell Univ. Ithaca, NY, United States)
de la Torre Juarez, M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Vasavada, A. R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Viudez-Moreiras, D.
(Centro de Astrobiología (CSIC-INTA) Madrid, Spain)
Zeitlin, C.
(Leidos, Inc. Houston, TX, United States)
Zorzano Mier, Maria-Paz
(Centro de Astrobiología (CSIC-INTA) Madrid, Spain)
Date Acquired
March 20, 2019
Publication Date
January 5, 2019
Publication Information
Publication: Geophysical Research Letters
Publisher: American Geophysical Union, Wiley
Volume: 46
Issue: 1
ISSN: 0094-8276
e-ISSN: 1944-8007
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
GSFC-E-DAA-TN66591
GSFC-E-DAA-TN65722
Report Number: GSFC-E-DAA-TN66591
Report Number: GSFC-E-DAA-TN65722
ISSN: 0094-8276
E-ISSN: 1944-8007
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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