Slide 1many different acceleration mechanisms: Fermi 1, Fermi 2, shear,... (Fermi acceleration at shock: most standard, nice powerlaw, few free parameters) main signatures…
1. www.DLR.de • Chart 1> IPIN 2013 > Patrick RobertsonSimultaneous Localization and Mapping for Pedestrians using Distortions of the Local Magnetic Field Intensity…
Modeling the Intermittent Dynamics of Alfvén Waves in the Solar Wind Abraham C.-L. Chian National Institute for Space Research (INPE), Brazil & Yohsuke Kamide (Nagoya…
Clusters of small eruptive flares produced by magnetic reconnection in the Sun. Clusters of small eruptive flares produced by magnetic reconnection in the Sun. Vasilis Archontis1…
Influence of solar wind density on ring current response R.S. Weigel George Mason University Geoeffectiveness â magnitude of a solar wind driver of geomagnetic activity…
Global coronal seismology and EIT waves Istvan Ballai SP2RC, University of Sheffield, UK Coronal seismology Local seismology: using waves propagating in magnetic structures…
many different acceleration mechanisms: Fermi 1, Fermi 2, shear, ... (Fermi acceleration at shock: most standard, nice powerlaw, few free parameters) main signatures to be…