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25 Years of Self-organized Criticality: Numerical Detection Methods |
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| Authors: | R T James McAteer Markus J Aschwanden Michaila Dimitropoulou Manolis K Georgoulis Gunnar Pruessner Laura Morales Jack Ireland Valentyna Abramenko |
| Institution: | 1. Solar Physics and Space Weather, Department of Astronomy, New Mexico State University, P.O. Box 30001, MSC 4500, Las Cruces, USA 2. Lockheed Martin, Solar and Astrophysics Laboratory (LMSAL), STAR Labs, A021S, Bldg. 252, 3251 Hanover St., Palo Alto, CA, 94304, USA 3. Dept. Physics, Kapodistrian University of Athens, 15483, Athens, Greece 4. Research Center Astronomy and Applied Mathematics, Academy of Athens, 4 Soranou Efesiou Street, 11527, Athens, Greece 5. Dept. Mathematics, Imperial College London, 180 Queen’s Gate, London, SW7 2AZ, United Kingdom 6. Departamento de Física, Facultad de Ciencias Exactas y Naturales, Instituto de Física Plasmas (CONICET), Universidad de Buenos Aires, Buenos Aires, Argentina 7. ADNET Systems, Inc., NASA Goddard Space Flight Center, MC. 671.1, Greenbelt, MD, 20771, USA 8. Space Weather Prediction Laboratory, Department of Solar Physics, Central Astronomical Observatory of Russian Academy of Science at Pulkovo, 65 Pulkovskoe Sh., St. Petersburg, 196140, Russia 9. Big Bear Solar Observatory of NJIT, 40386 N Shore Dr, Big Bear City, CA, 92314, USA |
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