Scientific motivation
1 Dwyer J R, Smith D M, Cummer S A, 2012 Space Sci Rev, DOI 10.1007/s11214-012-9894-0
1 Dwyer J R, Smith D M, Cummer S A, 2012 Space Sci Rev, DOI 10.1007/s11214-012-9894-0
BACKGROUND:
Studying of the High-energy Phenomena in the atmosphere is important for several reasons:
- It provides unique information about particle acceleration and multiplication in the lower and upper atmosphere during thunderstorms;
- Generation and propagation of huge fluxes of electrons, positrons, gammas and neutrons in the atmosphere and in space are newly discovered global processes that should be studied by experimental and theoretical methods;
- Electromagnetic emissions connected with thunderstorms trigger various dynamic processes in the Earth’s magnetosphere, causing global geo-effects and changing electrodynamics properties of the ionosphere.
- The large fluences of energetic electrons, photons and neutrons produced by runaway electron avalanches can potentially be a danger to individuals in aircraft.
GOALS AND STRUCTURE OF THE SYMPOSIUM:
The aim of the Symposium is two-fold:
1. To organize a large forum for discussing thunderstorm correlated observations of particle fluxes in the atmosphere and space and models of high energy phenomena originated in the atmosphere;
2. To discuss possible directions for the advancement in research, and for international cooperation between scientific groups using different experimental methods.
Based on these goals the following topics will be covered:
- Research of the Thunderstorm ground enhancements (TGEs), measurements of electrons, gamma rays and neutrons by networks of particle detectors located on Earth’s surface in correlation with thunderstorms;
- Research of the Terrestrial gamma-ray flashes (TGFs) observed by the orbiting gamma-ray observatories;
- Radio emissions produced by TGFs.
- Monitoring of thunderclouds from orbit;
- Methods of the remote sensing of the thunderstorm structure and electric field;
- Relation of the lightning occurrences to the TGE and TGF initiation;
- X-ray emissions from lightning;
- Relations to the climate and space weather issues;
- Possibility of joint observations by space-born and ground-based facilities.