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Origin, Injection, and Acceleration of CIR Particles: Theory Report of Working Group 7 |
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| Authors: | M Scholer G Mann S Chalov MI Desai LA Fisk JR Jokipii R Kallenbach E Keppler J Kóta H Kunow MA Lee TR Sanderson GM Simnett |
| Institution: | 1. Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany 2. Astrophysikalisches Institut Potsdam, Potsdam, Germany 3. Institute for Problems of Mechanics, Russian Academy of Sciences, Moscow, Russia 4. Dept. of Astronomy and IPST, University of Maryland, College Park, Maryland, USA 5. Dept. of Atmospheric and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA 6. Depts. of Planetary Sciences and Astronomy, University of Arizona, Tucson, Arizona, USA 7. International Space Science Institute, Bern, Switzerland 8. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany 9. Extraterrestrische Physik, Universit?t Kiel, Kiel, Germany 10. Space Science Center, University of New Hampshire, Durham, New Hampshire, USA 11. Space Science Dept. of ESA ESTEC, Noordwijk, The Netherlands 12. Physics and Astronomy Dept., University of Birmingham, Birmingham, United Kingdom |
| Abstract: | On the basis of the observational picture established in the report of Mason, von Steiger et al. (1999) the status of theoretical models on origin, injection, and acceleration of particles associated with Corotating Interaction Regions (CIRs) is reviewed. This includes diffusive or first-order Fermi acceleration at oblique shocks, adiabatic deceleration in the solar wind, stochastic acceleration in Alfvén waves and oblique propagating magnetosonic waves, and shock surfing as possible injection mechanism to discriminate pickup ions from solar wind ions. This revised version was published online in August 2006 with corrections to the Cover Date. |
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