YOU ARE HERE: Home

I want information on:

Information for:




MST5: Particle acceleration and transport at the Sun and in the heliosphere

Session Organisers:

Mykola Gordovskyy (University of Manchester, UK), N.Bian, V.Nakariakov

 

Acceleration of particles in flares and other explosive events and their transport in the solar atmosphere and heliosphere remains a major problem of solar and solar-terrestrial physics. Despite the significant progress made in the last decades, there are number of outstanding issues such as the mechanisms behind the huge numbers of non-thermal electrons derived from hard X-ray observations and the role of energetic ions in flares. In recent years, various space missions and ground-based instruments provided substantial volume of high-quality multi-wavelength data. The goal of this session is to review recent observational results and to discuss how to adopt theoretical models to the tight constrains imposed by these observations.

The session will focus on correlative analysis of simultaneous hard X-ray, gamma-ray and radio observations of non-thermal particles in the corona. In addition, we will discuss how to connect the results of remote and in-situ observations related to the high-energy particles in the heliosphere with the particle acceleration in the corona.

Although this session will concern the recent progress made in the field of particle acceleration at the Sun and transport in the heliosphere, it will also include a discussion of the role of future missions/instruments in solving the problem of energetic particles.

 

This is a complete listing of all 13 entries


Poster Session B
A classification scheme for stochastic acceleration  Nicolas Bian
The effect of turbulent density fluctuations on solar flare X-ray spectrum  Iain Hannah
Spatial properties of hard X-ray (HXR) coronal sources due to magnetic diffusion  Natasha Jeffrey
Effect of Langmuir wave diffusion on flare-accelerated electrons in the inhomogeneous coronal plasma  Heather Ratcliffe
the role of electron beam pitch angles and density gradients in solar Type III radio bursts  Roman Pechhacker
Influence of binary collisions on fast electrons in solar flares  Alec MacKinnon
Modelling Solar Energetic Particle Propagation for the COMESEP Alert System  Michael Marsh

Thursday 29th 11:45-13:00
11:45 Plasmoids in solar flares and their radio and X-ray diagnostics  Marian Karlicky
12:05 Long-Duration Solar Flares: Acceleration Without Heating  Ivan Zimovets
12:16 A solar burst with double radio spectrum observed up to 212 GHz  Paulo Simoes
12:27 Characteristics of flare acceleration regions using combined X-ray and Radio Observations  Hamish Reid
12:38 Particle Acceleration at Reconnecting 3D Null Points  Adam Stanier
12:49 Energetic particle diffusion in structured turbulence  Timo Laitinen