Mars Science Laboratory Observations of the 2018/Mars Year 34 Global Dust StormCollege of Engineering, University of Michigan, Ann Arbor, MI, USA.
Aeolis Research, Pasadena, CA, USA.
Department of Earth and Planetary Science, The Johns Hopkins University, Baltimore, MD, USA.
Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada.
Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada.
Centro de Astrobiología (INTA-CSIC), Madrid, Spain.
Finnish Meteorological Institute, Helsinki, Finland.
Southwest Research Institute, Boulder, CO, USA.
Department of Astronomy, University of Maryland, College Park, MD, USA.
Department of Earth and Space Science and Engineering, York University, Toronto, Ontario, Canada.
Finnish Meteorological Institute, , Helsinki, Finland; School of Electrical Engineering, Aalto University, , Espoo, Finland.
NASA Goddard Spaceflight Center, Greenbelt, MD, USA;CRESST II and Department of Astronomy, University of Maryland, College Park, MD, USA.
Aeolis Research, Pasadena, CA, USA.
NASA Goddard Spaceflight Center, Greenbelt, MD, USA.
Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY, USA.
Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY, USA.
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
Centro de Astrobiología (INTA-CSIC), Madrid, Spain.
Leidos, Houston, TX, USA.
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2019 (English)In: Geophysical Research Letters, ISSN 0094-8276, E-ISSN 1944-8007, Vol. 46, no 1, p. 71-79Article in journal (Refereed) Published
Abstract [en]
Mars 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‐nm optical depth reached 8.5, and Rover Environmental Monitoring Station measurements indicated a 97% reduction in incident total ultraviolet solar radiation at the surface, 30K reduction in diurnal range of air temperature, and an increase in the semidiurnal pressure tide amplitude to 40 Pa. 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.
Place, publisher, year, edition, pages
American Geophysical Union (AGU), 2019. Vol. 46, no 1, p. 71-79
National Category
Aerospace Engineering
Research subject
Atmospheric science
Identifiers
URN: urn:nbn:se:ltu:diva-72745DOI: 10.1029/2018GL080839ISI: 000456938600009Scopus ID: 2-s2.0-85059536242OAI: oai:DiVA.org:ltu-72745DiVA, id: diva2:1284284
Note
Validerad;2019;Nivå 2;2019-01-31 (johcin)
2019-01-312019-01-312019-10-10Bibliographically approved