Space weather forecasting Henrik Lundstedt Swedish Institute of Space Physics, Lund, Sweden .
LSE 2012 Extremes, Bursts and Mandelbrot's Eyes ... and Five Ways to Mis-estimate Risk
The Solar Wind-Polar Cap Interaction
ATMOP Partners Centre National de la Recherche Scientifique Centre National de la Recherche Scientifique (CNRS), France 7 th framework project selected.
IMF-dependent large-scale structure of plasma in the Earth's magnetotail - a study based on Prognoz-8 data Barbara Popielawska Space Research Center, PAS,
© NERC All rights reserved Storms rare but important Balance dataset otherwise storms look like noise Features selected like Split: training set, validation.
Identifying Coronal Holes in Solar Disk Images (and how to compare to models) Working Group Report Nick Arge Rachel Hock Carl Henney.
Space Physics Interactive Data Resource – SPIDR :Dr. ZHI N, Mik hail Dr. ZHI ZHI N, Mik hail (Ge oph ysic al Cen ter Rus sian Aca d. Sci. ) Dr. KIH N,
Five Spacecraft Observations of Oppositely Directed Exhaust Jets from a Magnetic Reconnection X-line Extending > 4.3 x 10 6 km in the Solar Wind Gosling.
Properties of Solar Wind ULF Waves Associated with Ionospheric Pulsations A D M Walker, & J A E Stephenson, & S Benz School of Physics University of KwaZulu-Natal.
EGU General Assembly 2011 Occurrence Frequency of Interplanetary Magnetic Flux Ropes K. Marubashi, Y.-H. Kim, K.-S. Cho, Y.-D. Park, K.-C. Choi, S. Choi,
Space Weather from Coronal Holes and High Speed Streams M. Leila Mays (NASA/GSFC and CUA) [email protected] SW REDISW REDI 2014 June 2-13.
