The Alfven-Carlquist double-layer theory of solar flares
Description
The Vlasov equations for ions and electrons are used to develop a theory of a double layer in which there are both free and trapped electrons and ions. The equations which replace the Langmuir condition and the Bohm conditions are found, and by numerically solving the resultant differential equation the authors find for particular choices of distribution functions the potential distribution in the layer. The applicability of this theory to solar flares is discussed, and it is shown that conditions in solar flares may be such that double layers can exist for which the free particles have a power-law energy distribution. These particles will be accelerated in a double layer and may in this way account for the production of high-energy particles during the impulsive phase of solar flares. (Auth.)
Additional details
Publishing Information
- Journal Title
- Astrophys. Space Sci.
- Journal Volume
- 56
- Journal Issue
- 1
- Series
- Astrophys. Space Sci.
- Journal Page Range
- 89-107
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 10424701
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BOLTZMANN-VLASOV EQUATION; DISTRIBUTION FUNCTIONS; ELECTRONS; HARD X RADIATION; IONS; NUMERICAL SOLUTION; POISSON EQUATION; SOLAR FLARES; SUN
- Descriptors DEC
- CHARGED PARTICLES; DIFFERENTIAL EQUATIONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; IONIZING RADIATIONS; LEPTONS; MAIN SEQUENCE STARS; RADIATIONS; SOLAR ACTIVITY; STARS; X RADIATION