Nonlinear Collisionless Perpendicular Diffusion of Charged Particles

By William H. Matthaeus, Gang Qin, J. Bieber, Gary Zank. 2003

460 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/9b31c75fcc0d1db1badd3e93e2b0a70e04a953a1

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. William H. Matthaeus
2. Huirong Yan
3. M. Potgieter
4. A. Strong
5. Gang Qin
6. A. Shalchi
7. A. Lazarian
8. Gary Zank

In Nuclear and High Energy Physics

1. A. Strong
2. Huirong Yan
3. M. Potgieter
4. Igor V. Moskalenko
5. A. Lazarian
6. A. Marcowith
7. A. Bykov
8. R. Diehl

Citations in the corpus

• PROPAGATION OF SOLAR ENERGETIC PARTICLES IN THREE-DIMENSIONAL INTERPLANETARY MAGNETIC FIELDS (2009, background): “Theoretical studies also show that nonlinear effects could cause large perpendicular diffusion (Matthaeus et al. 2003; Shalchi et al. 2004; Qin 2007).”
• Nonlinear Parallel and Perpendicular Diffusion of Charged Cosmic Rays in Weak Turbulence (2004, methodology): “So far only the nonlinear guiding center (NLGC) theory (Matthaeus et al. 2003; Shalchi et al. 2004) is able to describe cosmic-ray transport perpendicular to the magnetic background field.”
• Cosmic-Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field (2007, background): “For instance, it fails in treating 90o scattering (see Jones, Birmingham & Kaiser 1973, 1978; Völk 1973, 1975; Owens 1974; Goldstein 1976; Felice & Kulsrud 2001) and perpendicular transport (see Kóta & Jokipii 2000, Matthaeus et al. 2003).”
• ANISOTROPIC THREE-DIMENSIONAL FOCUSED TRANSPORT OF SOLAR ENERGETIC PARTICLES IN THE INNER HELIOSPHERE (2010, background): “…the above effects but also takes into account the complexity of the random magnetic field in directions transverse to the mean field was developed (Matthaeus et al. 2003) and applied with some success to the modulation of galactic cosmic rays and the results of numerical simulations of particle…”
• Particle acceleration at perpendicular shock waves: Model and observations (2005, background): “The frequently quoted value of l2D/lslab ’ 0.1 [e.g., Matthaeus et al., 2003, and references therein] is interesting in that it yields a very high injection threshold in the neighborhood of 90 , and the 90 value is still 4–5 orders of magnitude higher than at the corresponding parallel shock.”
• Solar Modulation of Cosmic Rays (2013, background): “Later, a new theory with different assumption, was developed by Matthaeus et al. (2003) and Bieber et al. (2004).”
• The origin of galactic cosmic rays (2013, unknown): “…however, not yet completely understood: the theory that currently best describes particle diffusion perpendicular to field lines was formulated by Matthaeus et al. (2003), and shows how the perpendicular diffusion coefficient depends in a non-trivial way upon the parallel diffusion coefficient,…”
• Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation (2016, background): “Perpendicular diffusion (Matthaeus et al. 2003) and field-line random walk (Giacalone et al. 2000) also contribute to escape.”
• The 511 keV emission from positron annihilation in the Galaxy (2010, background): “In particular, while non-linear effects were shown to be essential for particle transport in MHD turbulence (e.g. le Roux and Webb, 2007; Matthaeus et al., 2003; Zank et al., 2004), test-particle simulations of the coefficient Dpp do not exist at present.”