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Venus: Atmospheric Motion and Structure from Mariner 10 Pictures

Murray, Bruce C. and Belton, Michael J. S. and Danielson, G. Edward and Davies, Merton E. and Gault, Donald and Hapke, Bruce and O'Leary, Brian and Strom, Robert G. and Suomi, Verner and Trask, Newell (1974) Venus: Atmospheric Motion and Structure from Mariner 10 Pictures. Science, 183 (4131). pp. 1307-1315. ISSN 0036-8075. https://resolver.caltech.edu/CaltechAUTHORS:20151112-122053233

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Abstract

The Mariner 10 television cameras imaged the planet Venus in the visible and near ultraviolet for a period of 8 days at resolutions ranging from 100 meters to 130 kilometers. The general pattern of the atmospheric circulation in the upper tropospheric/lower stratospheric region is displayed in the pictures. Atmospheric flow is symmetrical between north and south hemispheres. The equatorial motions are zonal (east-west) at approximately 100 meters per second, consistent with the previously inferred 4-day retrograde rotation. Angular velocity increases with latitude. The subsolar region, and the region downwind from it, show evidence of large-scale convection that persists in spite of the main zonal motion. Dynamical interaction between the zonal motion and the relatively stationary region of convection is evidenced by bowlike waves.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.183.4131.1307DOIArticle
http://www.sciencemag.org/content/183/4131/1307.abstractPublisherArticle
http://www.jstor.org/stable/1737503JSTORArticle
Additional Information:© 1974 American Association for the Advancement of Science. 4 March 1974. We acknowledge the ingenuity, diligence, and dedication of the many engineers and scientists of the Jet Propulsion Laboratory who have contributed to the Mariner 10 television experiment. In particular the skilled staff of the Space Photography Section, the Image Processing Laboratory, the Mission Test Computer, and the Mission Test Information System have played a major role in our work. James Anderson and Michael Malin of the California Institute of Technology, Robert Krauss of the University of Wisconsin, and Ken Klaasen and Robert Toombs of the Jet Propulsion Laboratory made major contributions. It has been a special privilege to work with Gene Giberson, manager of the Mariner-Venus-Mercury Project, and his able staff. Andrew Ingersoll of the California Institute of Technology supplied valuable criticism. Contribution No. 2458 of the Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena 91109. Research sponsored in part by NASA contract NAS 7-100. Kitt Peak National Observatory is operated by AURA, Inc., under contract to the National Science Foundation.
Funders:
Funding AgencyGrant Number
NASANAS 7-100
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences2458
Issue or Number:4131
Record Number:CaltechAUTHORS:20151112-122053233
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20151112-122053233
Official Citation:Venus: Atmospheric Motion and Structure from Mariner 10 Pictures Bruce C. Murray, Michael J. S. Belton, G. Edward Danielson, Merton E. Davies, Donald Gault, Bruce Hapke, Brian O'Leary, Robert G. Strom, Verner Suomi, and Newell Trask Science 29 March 1974: 183 (4131), 1307-1315. [DOI:10.1126/science.183.4131.1307]
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:62073
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:13 Nov 2015 22:20
Last Modified:03 Oct 2019 09:15

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