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McEwen, A.1
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4
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0342355709
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note
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3 and some other S-compounds can be ruled out as major components based on the spectral data in the literature.
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7
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85040847975
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Springer-Verlag, Berlin
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_ and H.-U. Schmincke, Pyroclastic Rocks (Springer-Verlag, Berlin, 1984), pp. 263-254.
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Schmincke, H.-U.1
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0039825162
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Studies in Geophysics National Academy Press, Washington, DC, chap. 12
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K. Wohletz and R. McQueen, in Explosive Volcanism: Inception, Evolution, and Hazards, Studies in Geophysics (National Academy Press, Washington, DC, 1984), chap. 12.
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Wohletz, K.1
McQueen, R.2
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12
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0343225306
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note
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If the lava flows in the western delta were thinner than 1 m, they could not produce the extensive sheet flows observed in the 124 and 127 SSI images (1). If they were much thicker than 100 m, shadowed scarps would be visible at the flow margins. Based on the interpretation that the Prometheus lavas are inflated pahoehoe (1), and observations of similar inflated flows in the same size range on Earth, we suggest that the thickness of warm lava in the Prometheus lava "delta" is likely to be a few tens of meters.
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13
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0343660934
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note
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We have based the density estimate on the assumption that the observed high temperatures for the lava flows (2) indicate a lava of mafic, that is, relatively dense, composition.
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14
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0003897291
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Dover, New York
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-1. Under the fortuitous conditions considered here, the latent heat supplied by crystallization of the lava is almost exactly equal to the heat required for melting of the snow and the terms cancel in the conservation equations [M. Necati Ozisik, Boundary Value Problems of Heat Conduction (Dover, New York, 1968)]. Thermal conductivity could be appreciably lower if the lava is porous, or if temperatures are extremely high, perhaps by an order of magnitude. Lower values of thermal conductivity would extend the time scales calculated here.
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(1968)
Boundary Value Problems of Heat Conduction
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Ozisik, M.N.1
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15
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0001699135
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B. A. Smith, E. M. Shoemaker, S. W. Kieffer, A. F. Cook II, Nature 280, 738 (1979).
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Nature
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Smith, B.A.1
Shoemaker, E.M.2
Kieffer, S.W.3
Cook A.F. II4
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16
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0039825163
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D. Morrison, Ed. Univ. of Arizona Press, Tucson, AZ, fig. 18.5
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S. W. Kieffer, in Satellites of Jupiter, D. Morrison, Ed. (Univ. of Arizona Press, Tucson, AZ, 1982), fig. 18.5, p. 17.
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Satellites of Jupiter
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Kieffer, S.W.1
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17
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0040417715
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Clarendon, Oxford, ed. 2
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H. S. Carslaw and J. C. Jaeger, Conduction of Heat in Solids (Clarendon, Oxford, ed. 2, 1959), p. 88.
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Conduction of Heat in Solids
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Carslaw, H.S.1
Jaeger, J.C.2
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0040417714
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D. Morrison, Ed. Univ. of Arizona Press, Tucson, AZ
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T. V. Johnson and L. A. Soderblom, in Satellites of Jupiter, D. Morrison, Ed. (Univ. of Arizona Press, Tucson, AZ, 1982), chap. 17, p. 637.
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Johnson, T.V.1
Soderblom, L.A.2
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23
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0342790729
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note
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Portions of this work were performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. We also thank T. Johnson for pointing out that we had Prometheus bound if we had a mechanism to stop the motion of the plume.
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