The conversion of energy generated in the Sun's interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from th
Energy-dependent ionization states of shock-accelerated particles in the solar corona
β Scribed by Reames, D. V.; Ng, C. K.; Tylka, A. J.
- Book ID
- 118137270
- Publisher
- American Geophysical Union
- Year
- 1999
- Tongue
- English
- Weight
- 434 KB
- Volume
- 26
- Category
- Article
- ISSN
- 1944-8007
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The Conversion Of Energy Generated In The Sun's Interior Creates Its Hot Corona And A Wealth Of Dynamical Phenomena Such As Flares And Mass Ejections. Based On Recent Significant Progress In Understanding Magnetic Reconnection And A Wealth Of New Observations Of Energetic Particle Signatures From Th
Effective acceleration of particles by hydromagnetic turbulence requires that the particles be scattered at a rate v comparable with the frequency o9 of the turbulence. The only effective scattering process is due to resonant wave-particle interactions. The resonant waves are HM waves for ions with