Wednesday, May 17, 2017

Time Event  
10:30 - 11:00 Coffee break  
11:00 - 11:45 Decay Times for Interplanetary Type III : observations & simulations" - Milan Maksimovic  
11:45 - 12:30 Long duration energetic particle signatures in the solar corona - Ludwig Klein  
12:30 - 14:00 Lunch  
14:00 - 14:45 Solar Radio U-bursts and J-bursts observed with LOFAR Imaging Spectroscopy - Hamish Reid  
14:45 - 15:30 Using LOFAR to analyse the 16/04/2015 event - Thomas Murat  
15:30 - 16:15 Imaging Spectroscopy of a Type II solar radio burst observed by LOFAR - Nicolina Chrysaphi,  
16:15 - 16:45 Coffee break  
16:45 - 17:30 LOFAR observations of a giant loop in the outer corona - Mikola Gordovskyy,  
17:30 - 18:15 Turbulence and Standard Flare Model - Eduard Kontar  

Thursday, May 18, 2017

Time Event  
09:00 - 09:45 The role of diffusion in the transport of energetic electrons during solar flares - Nicolas Bian  
09:45 - 10:30 Particle acceleration in magnetic island formation and coalescence - Philippa Browning  
10:30 - 11:00 Coffee break  
11:00 - 11:45 Hybrid MHD/drift-kinetic modelling of mildly non-thermal plasma - Mykola Gordovskyy  
11:45 - 12:30 A physically-based sandpile model for the prediction of solar flares using data assimilation - - Antoine Strugarek  
12:30 - 14:00 Lunch  
14:00 - 15:00 Conclusion - Discussion