STATISTICAL ANALYSIS OF DISCONTINUITIES IN SOLAR WIND ACE DATA AND COMPARISON WITH INTERMITTENT MHD TURBULENCE

By A. Greco, William H. Matthaeus, S. Servidio, P. Chuychai, P. Dmitruk. 2009

204 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/740df0cb910340d5e4fb23f8966e1fea75ba2f09

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. C. Chen
2. S. Bale
3. O. Alexandrova
4. M. Velli
5. William H. Matthaeus
6. L. Sorriso-Valvo
7. Manolis K. Georgoulis
8. T. Horbury

In Molecular Biology

1. C. Chen
2. M. Velli
3. Manolis K. Georgoulis
4. William H. Matthaeus
5. T. Horbury
6. S. Bale
7. Markus J. Aschwanden
8. S. Cranmer

Citations in the corpus

• 25 Years of Self-Organized Criticality: Solar and Astrophysics (2014, methodology): “This was also demonstrated with MHD simulations (Watkins et al. 2001; Greco et al. 2009a,b), and by cellular automaton simulations with correlations in the driver that produces a “colored” power spectrum (Sanchez et al. 2002).”
• Who Needs Turbulence? (2011, methodology): “2011) based on the identification of discontinuities using the PVI-statistic (Greco et al. 2009), Osman et al.”
• Solar Wind Turbulence and the Role of Ion Instabilities (2013, background): “However, the vast majority of structures have no such signature: are these also part of the structure of the solar wind (Borovsky 2008), or are they generated dynamically by the turbulence (Greco et al. 2009, 2012)?”