Convection and Substorms: Paradigms of Magnetospheric Phenomenology eBook

Delivery: Can be download immediately after purchasing. For new customer, we need process for verification from 30 mins to 12 hours.
Version: PDF/EPUB. If you need EPUB and MOBI Version, please contact us.
Compatible Devices: Can be read on any devices.

The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth’s magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region. Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur. Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.

This is a digital product.

Convection and Substorms: Paradigms of Magnetospheric Phenomenology is written by Charles F. Kennel and published by Oxford University Press. The Digital and eTextbook ISBNs for Convection and Substorms are 9780195359077, 0195359070 and the print ISBNs are 9780195085297, 0195085299.