When you are asked to simulate the flow of gas in some corner of the universe, the first thing you need is a system of equations that govern the same. But let’s just say you have found yourself a closed, well posed system of equations, what next? The next choice one has to make is […]
To mesh or not to mesh? Read More »
The introduction of density and internal energy floors is seemingly unphysical, but at the same time, a necessary feature of General-Relativistic Magnetohydrodynamic simulations. The open magnetic field lines in the polar regions of our code that thread the black hole Event Horizon become devoid of any matter/energy due to the outflow boundaries at the inner
A lot of what we interpret from our astronomical telescopes is either through images/videos or raw data rendered understandable through physical plots in real or Fourier spaces. But what if we can render that data to cater to the other human senses? In this blog article I discuss very briefly the mechanics of data sonification
Understanding data through other senses: Data Sonification Read More »
