activity
20172024
most citedMulti-channel coronal hole detection with convolutional neural networks

38 citations · 231 across the 11 of their papers we have counts for

collaborators

18 papers

astro-ph.SR202215 cited

Multi-instrument STIX microflare study

J. Saqri, A. M. Veronig, A. Warmuth +7

During its commissioning phase in 2020, the Spectrometer/Telescope for Imaging X-rays (STIX) on board the Solar Orbiter spacecraft observed 69 microflares. The two most significant…

astro-ph.SR202138 cited

Multi-channel coronal hole detection with convolutional neural networks

R. Jarolim, A. M. Veronig, S. Hofmeister +4

We develop a reliable, fully automatic method for the detection of coronal holes, that provides consistent full-disk segmentation maps over the full solar cycle and can perform in…

q-fin.ST20211 cited

The value of big data for analyzing growth dynamics of technology based new ventures

Maksim Malyy, Zeljko Tekic, Tatiana Podladchikova

This study demonstrates that web-search traffic information, in particular, Google Trends data, is a credible novel source of high-quality and easy-to-access data for analyzing tec…

astro-ph.SR2021

Medium-term predictions of F10.7 and F30 cm solar radio flux with the adaptive Kalman filter

Elena Petrova, Tatiana Podladchikova, Astrid M. Veronig +3

The solar radio flux at F10.7 cm and F30 cm is required by most models characterizing the state of the Earth's upper atmosphere, such as the thermosphere and ionosphere to specify…

astro-ph.SR2020

Image Quality Assessment for Full-Disk Solar Observations with Generative Adversarial Networks

Robert Jarolim, Astrid Veronig, Werner Pötzi +1

In order to assure a stable series of recorded images of sufficient quality for further scientific analysis, an objective image quality measure is required. Especially when dealing…

astro-ph.SR202030 cited

Solar Flare-CME Coupling Throughout Two Acceleration Phases of a Fast CME

Tingyu Gou, Astrid M. Veronig, Rui Liu +8

Solar flares and coronal mass ejections (CMEs) are closely coupled through magnetic reconnection. CMEs are usually accelerated impulsively within the low solar corona, synchronized…