Who Needs Turbulence?

By William H. Matthaeus, M. Velli. 2011

205 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/a39d736091cee9e8f5e189c1b1a4733d5180ede9

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In Astronomy and Astrophysics

1. S. Cranmer
2. William H. Matthaeus
3. Gary Zank
4. S. Gibson
5. Don B. Melrose
6. Pete Riley
7. N. Lugaz
8. P. Isenberg

Citations in the corpus

• Alfvén Waves in the Solar Atmosphere (2012, background): “Magnetic reconnection is also observed in simulations of MHD turbulence (Matthaeus & Velli 2011; Rappazzo et al. 2008).”
• Coherent emission mechanisms in astrophysical plasmas (2017, methodology): “The turbulence in the IPM is consistent with a Kolmogorov spectrum (Matthaeus and Velli, 2011; Chen et al, 2012), which involves a turbulent cascade from larger to smaller scales.”
• Interstellar Mapping and Acceleration Probe (IMAP): A New NASA Mission (2018, background): “The ∼ 1-minute timescale extends into the dissipation range of turbulence (e.g., Matthaeus and Velli 2011) and is needed to separate discrete episodic events in contrast to continuously active processes in the production of suprathermal tails (e.g., Fisk and Gloeckler 2014; Schwadron et al. 1996).”
• Solar Wind Turbulence and the Role of Ion Instabilities (2013, unknown): “We shall restrict ourselves here to the solar wind turbulence, which is perhaps our best laboratory for studying astrophysical plasma turbulence (Tu and Marsch 1995; Bruno and Carbone 2005; Horbury et al. 2005; Matthaeus and Velli 2011).”
• Solar Modulation of Cosmic Rays (2013, background): “…turbulence effects in the heliosphere and on the fundamental process of reconnection and acceleration of particles, see Fisk and Gloeckler (2009, 2012), Lazarian et al. (2012), Lee et al. (2012), Matthaeus and Velli (2011), and several other contributions in the same issue of Space Science Reviews.”
• Origins of the Ambient Solar Wind: Implications for Space Weather (2017, background): “If there is a turbulent cascade that produces WTD-type heating, the ultimate energy dissipation may be best describable by small-scale reconnection events that reconfigure the magnetic topology (e.g., Matthaeus and Velli 2011).”