activity
20242026
collaborators

5 papers

astro-ph.SR2026

Quantifying the effect of passband on observations in the Ca II K line

Ajay Kumar Yadav, Theodosios Chatzistergos, Natalie Krivova +33

Full-disk observations of the Sun in the Ca II K line have been carried out since the late 19th century at various observatories worldwide. These long-term records of solar activit…

astro-ph.SR2025

Observations of the formation of a proto-spot in a pre-existing field environment

Mariarita Murabito, Ilaria Ermolli, Salvo L. Guglielmino +2

Bipolar emerging flux regions (EFRs) form active regions (ARs) that generally evolve in a pre-existing magnetic environment in the solar atmosphere. Reconfiguration of the small- a…

astro-ph.SR2025

Estimation of Polar Magnetic Fields using Ca II K Polar Network as a Proxy

Dibya Kirti Mishra, Bibhuti Kumar Jha, Theodosios Chatzistergos +3

The polar magnetic field plays a crucial role in the solar dynamo model and contributes to predicting future solar cycles. However, continuous and direct measurements of this polar…

astro-ph.SR2025

Ca II K Polar Network Index of the Sun: A Proxy for Historical Polar Magnetic Field

Dibya Kirti Mishra, Bibhuti Kumar Jha, Theodosios Chatzistergos +4

The Sun's polar magnetic field is pivotal in understanding solar dynamo processes and forecasting future solar cycles. However, direct measurements of the polar field is only avail…

astro-ph.SR2024

The Extreme Space Weather Event of 1872 February: Sunspots, Magnetic Disturbance, and Auroral Displays

Hisashi Hayakawa, Edward W. Cliver, Frédéric Clette +19

We review observations of solar activity, geomagnetic variation, and auroral visibility for the extreme geomagnetic storm on 1872 February 4. The extreme storm (referred to here as…