Journal article
Cross-scale physics and the acceleration of particles in collisionless plasmas throughout the Heliosphere and beyond: I. Collisionless shocks
Bulletin of the AAS, Vol.55(3), pp.1-6
07/31/2023
DOI: 10.3847/25c2cfeb.7f60730e
Abstract
Shocks in astrophysical plasmas are a fundamental, ubiquitous process considered responsible for accelerating many of the most energetic particles that we observe in the Universe, including galactic and anomalous cosmic rays (GCRs and ACRs) and solar energetic particles (SEPs). We present suggestions for focused, dedicated research of particle acceleration at shocks in the next decade.
Details
- Title: Subtitle
- Cross-scale physics and the acceleration of particles in collisionless plasmas throughout the Heliosphere and beyond: I. Collisionless shocks
- Creators
- Drew L. Turner - Johns Hopkins University Applied Physics LaboratoryLynn B. Wilson Iii - Goddard Space Flight CenterKaty Goodrich - West Virginia UniversityIan J. Cohen - Johns Hopkins University Applied Physics LaboratoryTerry Z. Liu - University of California, Los AngelesSteven J. Schwartz - University of Colorado SystemDamiano Caprioli - University of ChicagoColby Haggerty - University of Hawaii SystemImogen Gingell - University of SouthamptonMatt Hill - Johns Hopkins University Applied Physics LaboratoryElena Provornikova - Johns Hopkins University Applied Physics LaboratoryParisa Mostafavi - Johns Hopkins University Applied Physics LaboratoryPeter Kollmann - Johns Hopkins University Applied Physics LaboratoryPontus Brandt - Johns Hopkins University Applied Physics LaboratoryRalph McNutt - Johns Hopkins University Applied Physics LaboratoryBenoit Lavraud - Université de Bordeaux
- Resource Type
- Journal article
- Publication Details
- Bulletin of the AAS, Vol.55(3), pp.1-6
- DOI
- 10.3847/25c2cfeb.7f60730e
- Language
- English
- Date published
- 07/31/2023
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9985224314402771
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