1. To perform simulations of magnetic turbulence to investigate the topology of magnetic field lines and the orbits of energetic particles.
2. To use models of particle transport in turbulent magnetic fields to analyze data on solar energetic particles.
3. To work toward long-term monitoring of galactic cosmic rays at vertical cutoff rigidity 17 GV, including the establishment of the Princess Sirindhorn Neutron Monitor, analysis techniques, and theoretical studies of galactic cosmic ray anisotropy.
4. To provide Thai-language information on energetic particles in space, and space physics in general, to the community at large.
