Particle acceleration inside a 'gas' of shock waves

Details Particle acceleration inside a 'gas' of shock waves Particle acceleration inside a 'gas' of shock waves

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...245..271a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 245, no. 1, May 1991, p. 271-278.

Astronomy and Astrophysics

Astronomy

25

Magnetohydrodynamics, Particle Acceleration, Shock Waves, Solar Flares, Current Sheets, Magnetic Field Reconnection, Radio Jets (Astronomy), Shock Wave Interaction, Solar Radio Emission, Supernova Remnants

Scientific paper

A process by which shock waves are formed in jet flows or during
supernovae explosions is presented. Particular attention is given to the
short time scale evolution of N-shock wave-particle interaction. It is
found that most of the energy released by the 'thermal' explosions will
return to thermal energy via shock-shock interactions.

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