Utilizing many years of observation from deep space and near-earth spacecraft a theoretical understanding has evolved on how ions and electrons are accelerated in interplanetary shock waves. This understanding is now being applied to solar flare-induced shock waves propagating through the solar atmosphere. Such solar flare phenomena as gamma-ray line and neutron emissions, interplanetary energetic electron and ion events, and Type II and moving Type IV radio bursts appear understandable in terms of particle acceleration in shock waves.
Particle acceleration by coronal and interplanetary shock waves
1982-01-01
Miscellaneous
No indication
English
Particle acceleration by coronal and interplanetary shock waves
Elsevier | 1983
|Origin of Coronal and Interplanetary Shock and Particle Acceleration of a Flare/CME Event
British Library Conference Proceedings | 2003
|Origin of coronal and interplanetary shock and particle acceleration of a flare-CME event
Online Contents | 2003
|British Library Online Contents | 1992
|Solar and Interplanetary Particle Acceleration
British Library Conference Proceedings | 2003
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