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Hybrid simulations of rotational discontinuities1D hybrid simulations of rotational discontinuities (RDs) are presented. When the angle between the discontinuity normal and the magnetic field (theta-BN) is 30 deg, the RD broadens into a quasi-steady state of width 60-80 c/omega-i. The hodogram has a characteristic S-shape. When theta-BN = 60 deg, the RD is much narrower (10 c/omega-i). For right handed rotations, the results are similar to theta-BN = 30 deg. For left handed rotations, the RD does not evolve much from its initial conditions and the S-shape in the hodogram is much less visible. The results can be understood in terms of matching a fast mode wavelike structure upstream of the RD with an intermediate mode one downstream.
Document ID
19910068900
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Goodrich, C. C.
(Maryland Univ. College Park, MD, United States)
Cargill, P. J.
(Maryland, University College Park, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1991
Publication Information
Publication: Advances in Space Research
Volume: 11
Issue: 9 19
ISSN: 0273-1177
Subject Category
Astrophysics
Accession Number
91A53523
Funding Number(s)
CONTRACT_GRANT: NAG5-1101
Distribution Limits
Public
Copyright
Other

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