SH51B:
Intermittency and Dynamical Complexity in Space Plasmas from the Sun to Interplanetary and Planetary Environments I Posters
SH51B:
Intermittency and Dynamical Complexity in Space Plasmas from the Sun to Interplanetary and Planetary Environments I Posters
Intermittency and Dynamical Complexity in Space Plasmas from the Sun to Interplanetary and Planetary Environments I Posters
Session ID#: 2846
Friday, 19 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs: Marius Echim, Institute of Space Sciences, Bucharest, Romania and Giuseppe Consolini, INAF- Istituto di Astrofisica e Planetologia Spaziali, 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
