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20212025
most citedThe solar internetwork. III. Unipolar versus bipolar flux appearance

12 citations · 19 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025

Comparison of plasma dynamics in Coronal Holes and Quiet Sun using flux emergence simulations

Vishal Upendran, Durgesh Tripathi, Bhargav Vaidya +2

This paper presents a comparison of plasma dynamics in Coronal Holes (CHs) and Quiet Sun (QS) through 2.5D MHD flux emergence simulations. The magnetic reconnection between the eme…

astro-ph.SR2024★ 7 cited

Surface Flux Transport Modeling using Physics Informed Neural Networks

Jithu J Athalathil, Bhargav Vaidya, Sayan Kundu +2

Studying the magnetic field properties on the solar surface is crucial for understanding the solar and heliospheric activities, which in turn shape space weather in the solar syste…

astro-ph.IM2023

Quantifying Energy Release in Solar Flares and Solar Eruptive Events: New Frontiers with a Next-Generation Solar Radio Facility

Bin Chen, Dale E. Gary, Sijie Yu +16

Solar flares and the often associated solar eruptive events serve as an outstanding laboratory to study the magnetic reconnection and the associated energy release and conversion p…

astro-ph.IM2022

Towards data-driven modeling and real-time prediction of solar flares and coronal mass ejections

M. Rempel, Y. Fan, M. Dikpati +7

Modeling of transient events in the solar atmosphere requires the confluence of 3 critical elements: (1) model sophistication, (2) data availability, and (3) data assimilation. Thi…

astro-ph.SR2021★ 12 cited

The solar internetwork. III. Unipolar versus bipolar flux appearance

Milan Gošić, Luis R. Bellot Rubio, Mark C. M. Cheung +3

Small-scale internetwork (IN) magnetic fields are considered to be the main building blocks of the quiet Sun magnetism. For this reason, it is crucial to understand how they appear…