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On the dynamics in evaporating cloud envelopesCowie and McKee (1977) have conducted an analytical study of the case of an isolated, spherical cloud at rest in an infinite, hot medium. The present investigation is concerned with the theoretical model considered by Cowie and McKee for a thermally evaporating cloud. An analysis is conducted under the same conditions of inviscid flow with temperature equipartition. The current analysis allows for a continuous change in the saturation of the conductivity, rather than abrupt transitions from a classical to a fully saturated regime and back again, as in the model employed by Cowie and McKee. By suitable variable transformations, the momentum and energy equations can be reduced in the inviscid limit to a single equation for the Mach number in terms of a modified radius, and the solutions represented in a phase plane. An analytic model for the structure of the shock layer is developed.
Document ID
19840043156
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Giuliani, J. L., Jr.
(Princeton University New Observatory, Princeton, NJ, United States)
Date Acquired
August 12, 2013
Publication Date
February 15, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 277
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
84A25943
Funding Number(s)
CONTRACT_GRANT: NGL-31-001-007
Distribution Limits
Public
Copyright
Other

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