Solar X-ray and Radio Observations are complementary counterparts of the particle acceleration in a solar flare. Using Very Large Array Observations radio observations and RHESSI X-ray imaging and spectroscopy, we constraint conditions of particle acceleration. Now, we also add observations from various instruments onboard Parker Solar Probes and Solar Orbiter into the project.
Solar radio observations at meter wavelengths allow us to study various coronal diagnostic, including unique faint energetic releases. I use the solar data from Murchison Widefield Array, low freqeuncy precursor of SKA to investigate different solar science questions.
Studies related to Magneto-HydroDynamics (MHD)
Particle-in Cell Simulations