output
20162025
most citedSegmentation of coronal holes in solar disk images with a convolutional neural network

50 citations

Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2025

Low-Latitude Sunspot Group Tilt Angles in 15-24 Activity Cycles

Andrey Tlatov

An analysis of the tilt angles of the active regions in 15-24 activity cycles was performed. We used data from measurements of magnetic fields in the sunspot umbra in the period 19…

astro-ph.SR2019★ 36 cited

Peculiar solar sources and geospace disturbances on 20-26 August 2018

A. A. Abunin, M. A. Abunina, A. V. Belov +1

On the approach to minimum of Solar Cycle 24, on 26 August 2018, an unexpectedly strong geomagnetic storm (GMS) suddenly occurred. Its Dst index reached -174 nT, that is the third…

astro-ph.SR2019★ 22 cited

Reconstructing solar magnetic fields from historical observations V. Sunspot magnetic field measurements at Mount Wilson Observatory

Alexei A. Pevtsov, Kseniya A. Tlatova, Alexander A. Pevtsov +7

Context. Systematic observations of magnetic field strength and polarity in sunspots began at Mount Wilson Observatory (MWO), USA in early 1917. Except for a few brief interruption…

astro-ph.SR2018★ 36 cited

Solar Eruptions, Forbush Decreases and Geomagnetic Disturbances from Outstanding Active Region 12673

I. M. Chertok, A. V. Belov, A. A. Abunin

Based on our tool for the early diagnostics of solar eruption geoeffectiveness (EDSEG tool; Chertok et al., 2013, 2015, 2017), we have analyzed space weather disturbances that occu…

astro-ph.SR2018★ 50 cited

Segmentation of coronal holes in solar disk images with a convolutional neural network

E. Illarionov, A. Tlatov

Current coronal holes segmentation methods typically rely on image thresholding and require non-trivial image pre- and post-processing. We have trained a neural network that accura…

astro-ph.SR2018★ 42 cited

Tilt of sunspot bipoles in Solar Cycles 15 to 24

Ksenia Tlatova, Andrey Tlatov, Alexei Pevtsov +7

We use recently digitized sunspot drawings from Mount Wilson Observatory to investigate the latitudinal dependence of tilt angles of active regions and its change with solar cycle.…

astro-ph.SR2018★ 9 cited

Long-Term Oscillations of Sunspots and a Special Class of Artifacts in SOHO(MDI) and SDO(HMI) Data

V. I. Efremov, A. A. Soloviev, L. D. Parfinenko +6

A specific type of artifacts, that originate due to displacement of the image of a moving object along the digital (pixel) matrix of receiver are analyzed in detail. The criteria o…

astro-ph.SR2016★ 4 cited

On the Asymmetric Longitudinal Oscillations of a Pikelner's Model Prominence

J. Kraskiewicz, K. Murawski, A. Solov'ev +1

We present analytical and numerical models of a normal-polarity quiescent prominence that are based on the model of Pikelner (Solar Phys. 1971, 17, 44 ). We derive the general anal…

astro-ph.SR2016★ 32 cited

Tilt Angles of Solar Filaments over the Period 1919-2014

A. G. Tlatov, K. M. Kuzanyan, V. V. Vasil'yeva

The spatial and temporal distributions of solar filaments were analyzed using data from the Meudon Observatory for the period 1919-2003 and the Kislovodsk Mountain Astronomical Sta…