collaborators

5 papers

astro-ph.SR2026

A universal scaling between damping time and period of quasi-periodic pulsations from solar EUV brightenings to X-ray stellar flares

Daye Lim, Tom Van Doorsselaere, Valery M. Nakariakov +5

Recent high spatial and temporal resolution extreme-ultraviolet (EUV) imaging observations have revealed that quasi-periodic pulsations (QPPs), a ubiquitous signature of impulsive…

astro-ph.SR2025

Co-existence of longitudinal and transverse oscillations in polar plumes observed with Solar Orbiter/EUI

Upasna Baweja, Vaibhav Pant, S. Krishna Prasad +6

Magnetohydrodynamic (MHD) waves play a key role in heating the solar corona and driving the solar wind. Recent observations have shown the presence of slow magneto-acoustic and Alf…

astro-ph.SR2025

Understanding the magnetic field and plasma- along umbral fan loops traced using 3-min slow waves

Ananya Rawat, Girjesh Gupta, Tom Van Doorsselaere +2

The plasma- is an important fundamental physical quantity in solar plasma physics, which determines the dominating process in the solar atmosphere, i.e., magnetic or thermodyna…

astro-ph.SR2025

Nonlinearity of 3 minute Slow Magnetoacoustic Waves in the Sunspot Umbral Atmosphere

Y. Sanjay, S. Krishna Prasad, R. Sych +1

Slow magnetoacoustic waves with a 3 minute period are upward-propagating waves traveling through the density-stratified umbral atmosphere. The decreasing density causes their ampli…

astro-ph.SR2025

Height-Dependent Slow Magnetoacoustic Wave Amplitude and Energy Flux in Sunspot Atmospheres

Y. Sanjay, S. Krishna Prasad, P. S. Rawat

Slow magnetoacoustic waves (SMAWs) have been considered in the past as a possible candidate for chromospheric heating. This study analyzes 20 active regions observed between 2012 a…