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Evidence of a primordial solar windA model is reviewed which requires a T Tauri 'wind' and at the same time encompasses certain early-object stellar features. The theory rests on electromagnetic induction driven by the 'wind'. Plasma confinement of the induced field prohibits a scattered field, and all energy loss is via ohmic heating in the scatterer (i.e., planetary objects). Two modes, one caused by the interplanetary electric field (transverse magnetic) and the other by time variations in the interplanetary magnetic field (transverse electric) are present. Parent body melting, lunar surface melting, and a primordial magnetic field are components of the proposed model.
Document ID
19750043933
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Sonett, C. P.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Solar wind three; Third Conference
Location: Pacific Grove, CA
Start Date: March 25, 1974
End Date: March 29, 1974
Accession Number
75A28005
Funding Number(s)
CONTRACT_GRANT: NGR-03-002-363
Distribution Limits
Public
Copyright
Other

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