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Production of Different Non-Thermal Electron Groups in Small Solar Flares*
Published online by Cambridge University Press: 12 April 2016
Extract
Using the measurements of impulsive solar X-rays made with the OGO-5 satellite to identify the flash phase electron acceleration in solar flares of Hα-importance ≲ 1, the satellite and ground based observations are analyzed to study the origin of the different groups of non-thermal electrons responsible for the impulsive X-ray, impulsive microwave, type III radio and interplanetary electron emission.
- Type
- Section V / The Solar Flare Plasma
- Information
- Copyright
- Copyright © Reidel 1972
Footnotes
Research supported by NASA under Contract NAS 5-9094.