Coronal Mass Ejections provides an introduction to the solar coronal mass ejection phenomena. Readers will find a discussion of both corona and interplanetary coronal mass ejections, while learning how to detect and extract data from them.

The book introduces the solar coronal mass ejection phenomena. This includes both those observed in the corona and those further from the Sun, known as interplanetary coronal mass ejections. We discuss the history and physics behind these phenomena, theories describing their launch and evolution, association with other solar eruptive phenomena, and methods employed for their detection and scientific data extraction. Instruments used for their study (past, present and future) are also discussed, along with their resulting space weather effects on Earth and other planets. The latter requires a description of the Earth's magnetosphere, which is also included. Coronal Mass Ejections brings together solar physics, heliospheric physics, and magnetospheric physics, three traditionally separate fields of study. The content is accessible to beginning graduate students who are trying to master difficult fundamental concepts.

Brings together solar physics, heliospheric physics, and magnetospheric physics, three traditionally separate fields of study Accessible to beginning graduate students who are trying to master difficult fundamental concepts Discusses instruments used for studying solar phenomena and space weather effects on Earth and other planets Includes supplementary material: sn.pub/extras

Autorentext

Dr. Timothy Howard is a Senior Research Scientist conducting space physics research at the Southwest Research Institute in Boulder, Colorado. He received his PhD in Space and Plasma Physics from the University of Newcastle (Australia) in 2003. He has been a Postdoctoral Research Fellow in Space Physics at the National Solar Observatory, Montana State University, and Solar Physics at the University of Birmingham (UK). He has published over 30 refereed publications in various astrophysics and solar science journals and has had work presented at over 50 national and international meetings.

Klappentext

In times of growing technological sophistication and of our dependence on electronic technology, we are all affected by space weather. In its most extreme form, space weather can disrupt communications, damage and destroy spacecraft and power stations, and increase radiation exposure to astronauts and airline passengers. Major space weather events, called geomagnetic storms, are large disruptions in the Earth's magnetic field brought about by the arrival of enormous magnetized plasma clouds from the Sun. Coronal mass ejections (CMEs) contain billions of tons of plasma and hurtle through space at speeds of several million miles per hour. Understanding coronal mass ejections and their impact on the Earth is of great interest to both the scientific and technological communities.

This book provides an introduction to coronal mass ejections, including a history of their observation and scientific revelations, instruments and theory behind their detection and measurement, and the status quo of theories describing their onset and evolution through the heliosphere. We present the story behind the life of a CME, from its magnetic field origins in the solar corona and photosphere to its eventual fate deep in the heliosphere. The intention is to provide an easily accessible resource for those who are seeking to learn more about this fascinating and crucial natural phenomenon.

Inhalt
Chapter 1: Introduction.- Chapter 2: History.- Chapter 3: Summary of Spacecraft.- Chapter 4: How We Observe CMEs.- Chapter 5: Geometry of CMEs and ICMEs.- Chapter 6: Radio Astronomical Techniques.- Chapter 7: Associated Phenomena.- Chapter 8: CME Onset and Initial Acceleration.- Chapter 9: CME Evolution.- Chapter 10: Interaction With the Earth and Other Planets - Contribution to Space Weather.- Chapter 11: Summary and Discussion.- Glossary.- Index.