A MAGNETIC RECONNECTION MECHANISM FOR THE GENERATION OF ANOMALOUS COSMIC RAYS

By J. Drake, Merav Opher, M. Swisdak, J. Chamoun. 2010

199 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/7ad6114283fa0f90ec6f51dc4a2825ae48d94b63

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In Astronomy and Astrophysics

1. L. Sironi
2. A. Spitkovsky
3. Gianfranco Brunetti
4. A. Lazarian
5. Hui Li
6. V. Petrosian
7. George Livadiotis
8. L. Fletcher

In Nuclear and High Energy Physics

1. L. Sironi
2. Gianfranco Brunetti
3. A. Spitkovsky
4. A. Lazarian
5. Hui Li
6. Fan Guo
7. Yi‐Hsin Liu
8. V. Petrosian

Citations in the corpus

• Solar Modulation of Cosmic Rays (2013, background): “…to an anticipated power-law, and the ACR fluxes simply continued to increase as the two Voyagers moved away from the TS. Magnetic reconnection (Drake et al., 2010; Lazarian and Opher, 2009) and different forms of stochastic acceleration (Fisk and Gloeckler, 2009; Strauss et al., 2010a) have…”
• Acceleration of primary and secondary particles in galaxy clusters by compressible MHD turbulence: from radio haloes to gamma-rays (2010, methodology): “The idea of particle acceleration in reconnection regions was recently applied to describe anomalous cosmic ray acceleration in Heliosphere (Lazarian & Opher 2009, Drake et al.2010) and acceleration of cosmic rays in heliotail (Lazarian & Desiati 2010).”
• SEPARATION OF THE INTERSTELLAR BOUNDARY EXPLORER RIBBON FROM GLOBALLY DISTRIBUTED ENERGETIC NEUTRAL ATOM FLUX (2011, background): “Drake et al. (2010) suggested that the sectored heliospheric magnetic field, which results from the flapping of the heliospheric current sheet, piles up as it approaches the heliopause, narrowing the current sheets that separate the sectors and triggering the onset of collisionless magnetic…”
• RELATIVISTIC RECONNECTION: AN EFFICIENT SOURCE OF NON-THERMAL PARTICLES (2014, result): “The slope is steeper for lower magnetizations (p ∼ 4 for σ = 1, solid and dotted black lines), approaching the result from earlier studies of nonrelativistic reconnection, that found poor acceleration efficiencies (Drake et al. 2010).”
• Recent Advances in Understanding Particle Acceleration Processes in Solar Flares (2011, methodology): “D simulations (Zeiler et al. 2002; Pritchett & Coroniti 2004; Drake et al. 2010) and produced either as a result of an advective electric field (see the first term in Equation 3.9) and/or by a gradient of the magnetic field component across the current sheet (seethe second term in Equation 3.9.”
• PARTICLE ACCELERATION AND PLASMA DYNAMICS DURING MAGNETIC RECONNECTION IN THE MAGNETICALLY DOMINATED REGIME (2015, methodology): “…mechanisms such as direct acceleration at X-line regions (Drake et al. 2005; Fu et al. 2006; Pritchett 2006; Oka et al. 2010; Huang et al. 2010) and Fermi-type acceleration in reconnection induced plasma flows within magnetic islands (Drake et al. 2006, 2010; Oka et al. 2010; Huang et al. 2010).”