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On the Predominance of Oblique Disturbances in the Supersonic Shear Flow Instability of the Geomagnetic Tail Boundary : Volume 10, Issue 4/5 (30/11/-0001)

By Mishin, V. V.

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Book Id: WPLBN0004019551
Format Type: PDF Article :
File Size: Pages 11
Reproduction Date: 2015

Title: On the Predominance of Oblique Disturbances in the Supersonic Shear Flow Instability of the Geomagnetic Tail Boundary : Volume 10, Issue 4/5 (30/11/-0001)  
Author: Mishin, V. V.
Volume: Vol. 10, Issue 4/5
Language: English
Subject: Science, Nonlinear, Processes
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Historic
Publication Date:
-0001
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

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Mishin, V. V. (-0001). On the Predominance of Oblique Disturbances in the Supersonic Shear Flow Instability of the Geomagnetic Tail Boundary : Volume 10, Issue 4/5 (30/11/-0001). Retrieved from http://hawaiilibrary.net/


Description
Description: Institute of Solar-Terrestrial Physics Russian Academy of Sciences, P.O. Box 4026, Irkutsk 664033, Russia. A study is made of the influence of the longitudinal magnetic field and density inhomogeneity on the supersonic shear flow instability at the magnetospheric tail boundary. It is shown that the most unstable are slow oblique (3D) disturbances, with a phase velocity approaching at a sufficiently large angle (with respect to the flow direction) the magnetosonic velocity. Their growth rate and spectral width are much larger than those of the usually considered longitudinal (2D) supersonic disturbances. The magnetic field reduces the compressibility effect and, unlike the subsonic case, has a noticeable destabilizing effect on the excitation of oblique disturbances.

Summary
On the predominance of oblique disturbances in the supersonic shear flow instability of the geomagnetic tail boundary

 

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