activity
20092024
most citedSignatures of Alfven waves in the polar coronal holes as seen by EIS/Hinode

120 citations · 440 across the 14 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2024

Multithermal apparent damping of slow waves due to strands with a Gaussian temperature distribution

Tom Van Doorsselaere, S. Krishna Prasad, Vaibhav Pant +2

Context. Slow waves in solar coronal loops are strongly damped. The current theory of damping by thermal conduction cannot explain some observational features.\n Aims. We investiga…

astro-ph.SR2018★ 10 cited

Twisting/Swirling Motions During a Prominence Eruption as seen from SDO/AIA

V. Pant, A. Datta, D. Banerjee +2

A quiescent prominence was observed at north-west limb of the Sun using different channels of Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO). We report…

astro-ph.SR2017★ 22 cited

First Imaging Observation of Standing Slow Wave in Coronal Fan loops

V. Pant, A. Tiwari, D. Yuan +1

We observe intensity oscillations along coronal fan loops associated with the active region AR 11428. The intensity oscillations were triggered by blast waves which were generated…

astro-ph.SR2016★ 8 cited

The effects of transients on photospheric and chromospheric power distributions

T. Samanta, V. M. J. Henriques, D. Banerjee +4

We have observed a quiet Sun region with the Swedish 1-meter Solar Telescope (SST) equipped with CRISP Imaging SpectroPolarimeter. High-resolution, high-cadence, H line scanning…

astro-ph.SR2015★ 20 cited

Detection of high frequency oscillations and damping from multi-slit spectroscopic observations of the corona

T. Samanta, J. Singh, G. Sindhuja +1

During the total solar eclipse of 11 July 2010, multi-slit spectroscopic observations of the solar corona were performed from Easter Island, Chile. To search for high-frequency wav…

astro-ph.SR2015★ 47 cited

Forward Modelling of Standing Slow Modes in Flaring Coronal Loops

D. Yuan, T. Van Doorsselaere, D. Banerjee +1

Standing slow mode waves in hot flaring loops are exclusively observed in spectrometers and are used to diagnose the magnetic field strength and temperature of the loop structure.…