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Using machine learning to infer Solar coronal heating
This article traces the origins of the coronal heating problem, and describes in vivid detail our efforts in resolving this through machine learning. This is a non-technical article based on our paper, but references have been appended for the interested...
Bar Buckling and Boxy/Peanut Bulges as the Tracer of Dark Matter Halo Shape
Galaxies reside in the deep potential of invisible matter called dark matter. Their dynamics is significantly affected by the distribution of dark matter around them. Distribution of dark matter around galaxies is usually known as dark matter halo. Most of...
Using GitHub for Academic Research
GitHub has become the go-to tool for software engineers across the world to keep their codes together and collaborate with each other. Being easy, seamless, and available on all the platforms makes it a brilliant choice indeed.
How strong is a neutron star's magnetic field?
Estimating the strength of the magnetic field of a neutron star in a binary star system ‘Cen X-3’
Deciphering The Mysteries of The Quiet Sun Explosions
XSM onboard Chandrayaan 2 observed the Sun during its minimum activity period in 2019-2020. Using this data, the researchers have for the first time detected a very large number of small scale explosions, called microflares, happening on the Sun. The...
Measuring the age of the Universe: An overview
A popular article exploring how the age of the Universe was calculated.
