collaborators

5 papers

astro-ph.CO2026

Fitting trends in quasar emission and absorption line redshifts

Netra K Subramanian, Prasad Subramanian, Nimisha G Kantharia

The spectrum of a quasar consists of a few emission lines whose wavelengths are shifted by similar redshifts and numerous absorption lines whose wavelengths are shifted by differen…

astro-ph.SR2026

Aditya-L1/VELC observations of CME associated broadening of 5303Å coronal emission line

K. Sasikumar Raja, V. Muthu Priyal, R. Ramesh +2

We present Aditya-L1/VELC spectroscopic observations of 5303Å coronal emission line widths before and after coronal mass ejections (CMEs) which showed coronal dimming. The sit \& s…

astro-ph.SR2026

Intermittent turbulent fluctuations in solar coronal mass ejections

Apurva Bhagat, Sumit Tambe, Debesh Bhattacharjee +1

Localised regions of high intensity fluctuations are known to be signatures of intermittency in fluid and plasma turbulence. We investigate such turbulent spots using near-Earth {\…

astro-ph.SR2025

Proton heating estimates from near-Earth observations of coronal mass ejections in solar cycle 24

Debesh Bhattacharjee, Prasad Subramanian, Saikat majumder +1

As solar coronal mass ejections (CMEs) propagate through the heliosphere, they expend energy in heating protons to compensate for the cooling that occurs due to expansion. CME prop…

astro-ph.SR2025

Turbulent power: a discriminator between sheaths and CMEs

Deep Ghuge, Debesh Bhattacharjee, Prasad Subramanian

Solar coronal mass ejections (CMEs) directed at the Earth often drive large geomagnetic storms. Here we use velocity, magnetic field and proton density data from 152 CMEs that were…