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From the 1 of 13 linked papers with an AI index.

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20242026
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13 papers

astro-ph.SR2026

Multi-Wavelength Diagnostics of Pre-Flare Evolution with Aditya-L1: From the Solar Chromosphere to the Corona

Adithya H. N., Sreejith Padinhatteeri, Soumya Roy +13

The pre-flare phase of solar flares provides important insight into the processes that drive active regions toward instability. We investigate chromospheric pre-flare activity usin…

astro-ph.IM2026

WALOP-South: a four camera one shot imaging polarimeter for the PASIPHAE survey. Paper III -- PSF modelling

Indrajit Paul, Kishan Deka, Tuhin Ghosh +22

The paper presents a polar shapelet‑based method for modeling the point spread function of the WALOP‑South wide‑field imaging polarimeter, achieving ~0.15% photometric accuracy for…

astro-ph.SR2026

Unraveling the Secrets of the lower Solar Atmosphere: One year of Operation of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1

Rahul Gopalakrishnan, Soumya Roy, Deepak Kathait +20

The Solar Ultraviolet Imaging Telescope (SUIT) is an instrument onboard Aditya--L1, the first solar space observatory of the Indian Space Research Organization (ISRO), India, launc…

astro-ph.GA2026

Evidence for cloud-to-cloud variations in the ratio of polarized thermal dust emission to starlight polarization

Nidhi Mehandiratta, Georgia V. Panopoulou, Eirik Gjerløw +12

The correlation between optical starlight polarization and polarized thermal dust emission can be used to infer intrinsic dust properties. This correlation is quantified by the rat…

astro-ph.IM2025

Wide Area Linear Optical Polarimeter Control Software

John A. Kypriotakis, Bhushan Joshi, Dmitry Blinov +19

The WALOPControl software is designed to facilitate comprehensive control and operation of the WALOP (Wide Area Linear Optical Polarimeter) polarimeters, ensuring safe and concurre…

astro-ph.SR2025

Zero-polarization candidate regions for calibration of wide-field optical polarimeters

N. Mandarakas, G. V. Panopoulou, V. Pelgrims +14

Context. Calibration of optical polarimeters relies on the use of stars with negligible polarization (unpolarized standard stars) for determining the instrumental polarization zero…