Bookcover of Magnetic field structure and evolution of flaring solar active regions
Booktitle:

Magnetic field structure and evolution of flaring solar active regions

LAP LAMBERT Academic Publishing (2016-09-15 )

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ISBN-13:

978-3-659-94398-0

ISBN-10:
3659943983
EAN:
9783659943980
Book language:
English
Blurb/Shorttext:
Solar Eruptions including flares, Coronal Mass Ejections (CMEs) are energetic, explosive transient events releasing enormous amounts of energy due to sudden destabilization of magnetic field in the active regions (ARs). Large flares and CMEs are primary causes of space-weather disturbances which include satellite failure, disruption of communication and power systems etc. Therefore, there is a need to better understand the underlying physics and associated phenomena in these eruptive events, and to refine the prediction capabilities that help in taking precautionary/preventive measures. This work deals with observational evidences for storing and releasing energy in the magnetic system of ARs where eruptions mostly occur. The prime observational data used in this study is from NASA's space-born Solar Dynamic Observatory. In this context, the study focuses on the triggering and driving mechanisms of eruptions, helicity and energy storage by field line foot point motions at the photosphere and methods of coronal magnetic field modeling using photospheric magnetic field observations.
Publishing house:
LAP LAMBERT Academic Publishing
Website:
https://www.lap-publishing.com/
By (author) :
Vemareddy Panditi
Number of pages:
160
Published at:
2016-09-15
Stock:
Available
Category:
Physics, astronomy
Price:
64.90 €
Keywords:
Corona, Helicity, magnetic fields, Reconnection, Solar Physics, Sun, flares, CMEs, space-weather

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