collaborators

9 papers

astro-ph.SR2026

Large ephemeral regions and their tilt angles

Rambahadur Gupta, Anu Sreedevi, Bibhuti Kumar Jha +1

The ephemeral regions (ERs), which are short-lived bipolar magnetic regions that emerge across the solar cycle but do not appear as sunspots, play a crucial role in the Sun's magne…

astro-ph.SR2026

Addressing Known Challenges in Solar Flare Forecasting I: Limb-Flare Prediction with a 4-pi Full-Heliosphere Framework

K. D. Leka, Eric L. Wagner, Lisa Upton +3

A demonstrated failure mode for operational solar flare forecasting is the inability to forecast flares that occur near, or just beyond, the solar limb. To address this shortcoming…

astro-ph.SR2025

Backtracking Bipolar Magnetic Regions to their emergence: Two groups and their implication in the tilt measurements

Anu Sreedevi, Bidya Binay Karak, Bibhuti Kumar Jha +2

Bipolar Magnetic Regions (BMRs) that appear on the solar photosphere are surface manifestations of the Suns internal magnetic field. With modern observations and continuous data st…

astro-ph.SR2025

Historical Reconstruction of Solar Surface Magnetism from Cycle 1-24 Using the Synthetic Active Region Generator (SARG) and the Advective Flux Transport (AFT) Model

Bibhuti Kumar Jha, Lisa A. Upton, Greg Kopp +1

The historical reconstruction of the Sun's surface magnetic field remains a persistent challenge, limiting our ability to investigate the long-term global properties of the Sun, in…

astro-ph.SR2025

Machine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts

Dibya Kirti Mishra, Subhamoy Chatterjee, Bibhuti Kumar Jha +6

Kodaikanal Solar Observatory (KoSO) is one of the oldest solar observatories, possessing an archive of multi-wavelength solar observations, including white light, Ca II K, and H-al…

astro-ph.SR2025

Observed Joys law of Bipolar Magnetic Region tilts at the emergence supports the thin flux tube model

Anu Sreedevi, Bidya Binay Karak, Bibhuti Kumar Jha +2

Bipolar sunspots, or more generally, Bipolar Magnetic Regions, BMRs, are the dynamic magnetic regions that appear on the solar surface and are central to solar activity. One striki…