Solar flares are powerful explosions in the solar system, releasing energy stored in nonpotential magnetic fields. They cause plasma heating, enhancing soft X-rays and longer-wavelength emissions. These flares, often associated with Coronal Mass Ejec
Section: Physical Sciences (Research Project)
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Constraining Solar
Constraining Solar Flare Height-Time Heating Profile and Energy Deposition Using Combined Multiwavelength Observations from Aditya–L1, Chandrayaan–2 and Numerical Simulations
Research Project › Mathematical Sciences
Unraveling ubiquitous
Unraveling ubiquitous small-scale magnetic reconnection in the solar lower atmosphere
Research Project › Physical Sciences
Unveiling the
Unveiling the hidden relationship between vorticity and magnetic field in the solar atmosphere
Research Project › Physical Sciences
Probing Relativistic
Probing Relativistic Jets Using Polarization of Blazar Emission
Research Project › Physical Sciences
Development of
Development of Signal processing algorithms for demonstration of Solar observations in microwave frequencies
Research Project › Mathematical Sciences
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