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Interannual variability of Mars' south polar cap
Institution:1. Laboratory for Atmospheric and Space Physics, University of Colorado, 3665 Discovery Drive, Boulder, CO 80303, USA;2. Department of Geological Sciences, University of Colorado, 399 UCB, Boulder, CO 80309, USA;3. Department of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK;4. Laboratoire de Planétologie et Géodynamique - UMR CNRS 6112, 2 rue de la Houssinière - BP 92208, 44322 Nantes Cedex 3, France;1. University of Hawai''i, Honolulu, HI, United States;2. Planetary Science Institute, Tucson, AZ, United States;3. Smithsonian Institution, Washington, DC, United States;4. Arizona State University, Tempe, AZ, United States;1. Department of Earth and Planetary Sciences, Washington University in Saint Louis, Saint Louis, MO 63130, USA;2. Max Planck Institute for Astrophysics, 85748 Garching bei München, Germany;3. Department of Electrical and Systems Engineering, Washington University in Saint Louis, Saint Louis, MO 63130, USA;4. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA;5. Space Science Institute, Boulder, CO 80301, USA
Abstract:Telescopic data on the twentieth-century regressions of Mars' south polar cap have been reexamined for evidence of interannual variability. Several regressions, particularly that of 1956, are found to differ significantly from the mean. The possibility of correlations with major dust storms is explored.
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