Published February 1989
| Version v1
Journal article
Minimum Mach number for impulsive proton acceleration by parallel collisionless shock waves in solar flares
Creators
- 1. Berkeley Research Associates, CA (USA)
- 2. Colorado Univ., Boulder (USA)
Description
A lower limit to the minimum Alfven Mach number M(A) is determined for which a parallel shock could accelerate protons to 10 MeV in 2 s for low coronal conditions in which the density is 9.5 x 10 to the 10th/cu cm, the magnetic field is 56 G, and the temperature is 1.6 x 10 to the 6th K. A lower limit to the time to generate the Alfven waves necessary to scatter the protons back to the shock where they can be accelerated by the shock compression is derived, and the upstream and downstream mean free paths are determined. The actual acceleration time after the Alfven waves are established. The lower limit to M(A) is 2.0. 16 references
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 337
- Series
- Astrophys. J.
- Journal Page Range
- 954-958
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20070612
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCELERATION; ALFVEN WAVES; DENSITY; GAMMA RADIATION; HYDROMAGNETIC WAVES; LIMITING VALUES; MACH NUMBER; MAGNETIC FIELDS; PLASMA; SHOCK WAVES; SOLAR CORONA; SOLAR FLARES; SOLAR PROTONS; WAVE PROPAGATION
- Descriptors DEC
- ATMOSPHERES; BARYONS; CATIONS; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONIZING RADIATIONS; IONS; NUCLEONS; PHYSICAL PROPERTIES; PROTONS; RADIATIONS; SOLAR ACTIVITY; SOLAR ATMOSPHERE; SOLAR PARTICLES; SOLAR RADIATION; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR FLARES; STELLAR RADIATION; VELOCITY