Abstract
Undoubtedly, the most lively manifestation of the dynamic nature of the earth’s magnetosphere is the auroral break-up. The magnetospheric phenomena that are associated with this explosive release of energy have been the aim of intense research efforts in recent years, and the term magnetospheric substorm has been introduced to designate these phenomena as a whole. The ‘polar magnetic substorm’ is the manifestation of the magnetospheric substorm in the polar magnetic field. Other aspects of the magnetospheric substorm are similarly called ‘auroral substorm,’ ionospheric substorm,’ etc. (Akasofu, 1968). The magnetospheric substorm represents a process in which plasma is accelerated and electric current is generated at the expense of the magnetic field energy stored in the magnetotail.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 1978 Springer Science+Business Media New York
About this chapter
Cite this chapter
Nishida, A. (1978). Implosion in the Magnetotail. In: Geomagnetic Diagnosis of the Magnetosphere. Physics and Chemistry in Space, vol 9. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-86825-2_3
Download citation
DOI: https://doi.org/10.1007/978-3-642-86825-2_3
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-86827-6
Online ISBN: 978-3-642-86825-2
eBook Packages: Springer Book Archive