SH52A:
Intermittency and Dynamical Complexity in Space Plasmas from the Sun to Interplanetary and Planetary Environments II
SH52A:
Intermittency and Dynamical Complexity in Space Plasmas from the Sun to Interplanetary and Planetary Environments II
Intermittency and Dynamical Complexity in Space Plasmas from the Sun to Interplanetary and Planetary Environments II
Session ID#: 4410
Friday, 19 December 2014: 10:20 AM-12:20 PM
2012 (Moscone West)
Chairs: Marius Echim, Institute of Space Sciences, Bucharest, Romania and Giuseppe Consolini, CNR National Institute for Astrophysics, Rome, Italy
Primary Convener: Marius Echim, Institute for Space Sciences, Magurele, Romania; Belgian Institute for Space Aeronomy, Brussels, Belgium
Co-conveners: Giuseppe Consolini, INAF- Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy and Tom Chang, Massachusetts Institute of Technology, Kavli Institute for Astrophysics and Space Research, Cambridge, MA, United States
OSPA Liaison: Zoltan Voros, Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Co-Sponsor(s):
- NG - Nonlinear Geophysics
- SA - SPA-Aeronomy
- SM - SPA-Magnetospheric Physics
Index Terms:
2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2756 Planetary magnetospheres [MAGNETOSPHERIC PHYSICS]
4440 Fractals and multifractals [NONLINEAR GEOPHYSICS]
4468 Probability distributions, heavy and fat-tailed [NONLINEAR GEOPHYSICS]
Virtual Option?: No
Swirl Theme: Convection and circulation across scales
Abstracts Submitted to this Session:
See more of: SPA-Solar and Heliospheric Physics
