collaborators

6 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.SR2026

Reconstruction of annual solar irradiance over the last three millennia

D. Temaj, N. A. Krivova, S. K. Solanki +2

Solar irradiance measurements are limited to the last few decades, requiring reconstructions to assess solar variability on longer timescales and its impact on Earth's climate. We…

astro-ph.SR2026

Empirical flare energy limits for the largest historical sunspots

N. A. Krivova, T. Chatzistergos, M. Kazachenko +1

Extreme solar particle events reveal that the Sun can occasionally produce eruptions significantly more energetic than those observed in the modern era. These events are thought to…

astro-ph.SR2026

Solar Irradiance Reconstruction over the Telescopic Era Using a Revised Photospheric Magnetic Field Model

D. Temaj, N. A. Krivova, T. Chatzistergos +2

The Sun is the primary source of energy for Earth and one of the main external drivers of its climate. Solar irradiance -- the radiative power emitted by the Sun and received at 1-…

astro-ph.SR2026

Quantifying sunspot group nesting with density-based unsupervised clustering

Nurdan Karapinar, Emre Isik, Natalie A. Krivova +1

Sunspot groups often emerge in spatial-temporal clusters, known as nests or complexes of activity. Quantifying how frequently such nesting occurs is important for understanding the…

astro-ph.SR2026

Linking Solar Magnetism, Extreme Solar Particle Events and Stellar Superflares

Valeriy Vasilyev, Natalie Krivova, Ilya Usoskin

The magnetic field of the Sun drives a wide range of eruptive phenomena, from small-scale nanoflares to large flares and coronal mass ejections (CMEs). While direct observations of…