The Common Spectrum for Accelerated Ions in the Quiet-Time Solar Wind
By L. Fisk, G. Gloeckler. 2006
209 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/79ef2334e93797022c1343e3d575918683906d82
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
- George Livadiotis
- S. Cranmer
- David John McComas
- S. Bale
- Gary Zank
- Justin C. Kasper
- V. Florinski
- D. Lario
Citations in the corpus
- Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus (2015, background): “…quasi-linear 2nd order Fermi acceleration and transit-time damping (Fisk et al. 1974; Miller 1998), and (b) non-resonant stochastic acceleration by turbulent fluid compressions and rarefactions (Ptuskin 1988; Webb et al. 2003; Le Roux et al. 2002; Cho and Lazarian 2006; Fisk and Gloeckler 2006).”
- The Solar Probe Plus Mission: Humanity’s First Visit to Our Star (2016, background): “Interchange reconnection models for solar wind generation explicitly assume an intrinsic intermittency at the solar wind source in the form of reconnection between open field lines and closed coronal loops (e.g., Fisk 1996; Schwadron and McComas 2003; Suess et al. 1998; Antiochos et al. 2010).”
- The Effects of a κ-Distribution in the Heliosheath on the Global Heliosphere and ENA Flux at 1 AU (2008, background): “More recently, with the measurement of PUIs byUlysses (Gloeckler et al. 2005; Fisk & Gloeckler 2006), it became apparent that the PUI distribution merged cleanly into the solar wind distribution, yielding an extended energetic tail.”
- SEPARATION OF THE INTERSTELLAR BOUNDARY EXPLORER RIBBON FROM GLOBALLY DISTRIBUTED ENERGETIC NEUTRAL ATOM FLUX (2011, methodology): “Prested et al. (2008, 2010) and Heerikhuisen et al. (2008) developed models of ENAs from the heliosheath using kappa distributions with an assumed value of κ ∼ 1.5 based on the observations of suprathermal ions in the solar wind of the inner heliosphere (Fisk & Gloeckler 2006).”
- Kappa Distributions: Theory and Applications in Space Plasmas (2010, background): “…statistical mechanics formulated fora collisionless plasmas far from thermal (Boltzmann-Maxwell) equilibrium but containing fully developed turbulence in quasistationary equilibrium (Treumann 1999a,b; Leubner 2002; Fisk and Gloeckler 2006; Gloeckler and Fisk 2006; Treumann and Jaroschek 2008).”