NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Dynamics of volcanic plumes on IoBallistic and aerodynamic models are proposed to explain the dynamics of the volcanic plumes on Io. A ballistic model, which assumes that eruptive gas and solid-particle flows become completely and permanently decoupled over a small distance as compared with the maximum particle height, is shown to be unable to account for the observed shape of Plume 3. An aerodynamic model which assumes the entrainment and transportation of solid particles by the gas flow into the central portion of the top of the plume, with ballistic particle trajectories only after passage through the first part of their descent, is then developed. The model accounts for plume shape by the formation of a weak decompression shock near the edge of the plume stalk, which constrains horizontal expansion until a sufficient altitude is reached. Calculated plume dimensions are then compared with observations of Ionian Plumes 1 and 3.
Document ID
19790064779
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cook, A. F.
(Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Shoemaker, E. M.
(U.S. Geological Survey Flagstaff, Ariz., United States)
Smith, B. A.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
August 30, 1979
Publication Information
Publication: Nature
Volume: 280
Subject Category
Lunar And Planetary Exploration
Accession Number
79A48792
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available