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Pulsars and Bubble Dynamics

Published online by Cambridge University Press:  12 April 2016

Ramen Kumar Parui
Ramen Kumar Parui*
Affiliation:
Aero Communication Station (ACS), Imphal Airport, P.O.-Tulihal, Imphal-795140, India

Abstract

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Based on recent observation of the dominance of the flare generated solar wind streams over the co-rotating streams and a significant lowering in the cosmic ray intensity in the abnormal year of the solar activity period, I have predicted the occurrence of discernible changes in magnetic field strength and the thickness of the shell of the local bubble during high sunspots years of the solar cycle period. In order to observe the variation, both in the magnetic field strength and in the thickness of the compressed shell, a proposal of continuous monitor of these two parameters through the observation of Faraday Rotation Measure has been proposed with an emphasize to the observations in the period of next abnormal year of the solar cycle in near future.

Type
Part IV Clouds, Ionized Gas, and Particles in the Local ISM
Information
International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 223 - 226
Copyright
Copyright © Springer-Verlag 1998

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