Magnetic Field Amplification by Shocks in Turbulent Fluids

By J. Giacalone, J. Jokipii. 2007

262 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/90d6263eb2c0e22368ff55b6781b10afb4af5ccc

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. Y. Fukui
2. Tsuyoshi Inoue
3. S. Inutsuka
4. T. W. Jones
5. R. Yamazaki
6. Hyesung Kang
7. Y. Ohira
8. D. Ryu

In Nuclear and High Energy Physics

1. Y. Fukui
2. Tsuyoshi Inoue
3. S. Inutsuka
4. T. W. Jones
5. Hyesung Kang
6. Y. Ohira
7. D. Ryu
8. R. Yamazaki

Citations in the corpus

• DIFFUSIVE SHOCK ACCELERATION SIMULATIONS OF RADIO RELICS (2012, background): “In addition, magnetic fields can be amplified by turbulent motions behind shocks (Giacalone & Jokipii 2007; Inoue et al. 2009).”
• The origin of galactic cosmic rays (2013, unknown): “In addition to the CR-induced instabilities discussed above, there are also fluid instabilities (e.g. see Giacalone and Jokipii 2007) that only amplify magnetic field downstream of the shock if a density inhomogeneity is present upstream on suitably chosen scales.”
• TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM (2009, background): “Recently Giacalone & Jokipii (2007) have demonstrated by using magnetohydrodynamic (MHD) simulation that density fluctuations in the preshock medium cause turbulence and magnetic field amplification in the postshock medium.”
• Gamma-rays from molecular clouds illuminated by cosmic rays escaping from interacting supernova remnants (2010, background): “…the shock is studied by the linear analysis (Bell 2004; Reville et al. 2007; Ohira et al. 2009b) and many numerical simulations (Lucek & Bell 2000; Giacalone & Jokipii 2007; Niemiec et al. 2008; Reville et al. 2008; Riquelme & Spitkovsky 2009; Inoue et al. 2009; Ohira et al. 2009a; Vladimirov et…”
• TOWARD UNDERSTANDING THE COSMIC-RAY ACCELERATION AT YOUNG SUPERNOVA REMNANTS INTERACTING WITH INTERSTELLAR CLOUDS: POSSIBLE APPLICATIONS TO RX J1713.7−3946 (2011, background): “The turbulence induced by the shock-cloud interactions amplifies the magnetic field through turbulent dynamo actions (see also, Balsara et al. 2001; Giacalone & Jokipii 2007), which potentially account for the year-scale short-time variability of X-rays in RX J1713.”