Colby Haggerty
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Modeling the saturation of the Bell instability using Hybrid simulations (Submitted)

Modeling the saturation of the Bell instability using Hybrid simulations (Submitted)

by Colby Haggerty | Jan 22, 2024 | Uncategorized

G. Zacharegkas, D. Caprioli, C. C. Haggerty, S. Gupta and B. Schroer Abstract: The nonresonant streaming instability (Bell instability) plays a pivotal role in the acceleration and confinement of cosmic rays (CRs); yet, the exact mechanism responsible for its...

Recent Posts

  • Modeling the saturation of the Bell instability using Hybrid simulations (Submitted)
  • The Importance of Heat Flux in Quasi-Parallel Collisionless Shocks (Submitted)
  • Relativistic Asymmetric Reconnection (2022)
  • Ion Acceleration Efficiency at the Earth’s Bow Shock: Observations and Simulation Results (2021)
  • Kinetic Simulations of Cosmic-Ray-Modified Shocks II: Particle Spectra (2020)

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Institute for Astronomy
University of Hawaiʻi at Mānoa
2680 Woodlawn Dr, Rm. B109
Honolulu, HI 96822

ColbyH [at] hawaii.edu

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