activity
20142026
most citedSolar polar brightening and radius at 100 and 230 GHz observed by ALMA

29 citations · 52 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2026

The energetic atmosphere of the Sun

Sven Wedemeyer, Mats Kirkaune, Miroslav Barta +16

Understanding the mechanisms that heat the Sun's chromosphere and corona to temperatures far exceeding those of the solar photosphere below remains one of the central challenges in…

astro-ph.SR2026

Delayed, Line-dependent Reorganization of Pore Oscillations Following a Compact C8.2 Flare Observed by Sunrise III/SUSI

Shahin Jafarzadeh, David B. Jess, Marco Stangalini +34

Magnetic oscillations permeating the solar atmosphere can be altered by flares. This could be due to changes in the atmospheric magnetic waveguide, the thermodynamic stratification…

astro-ph.IM2026

Voltage-to-temperature calibration of the High Altitude THz Solar telescope acquisition system

Gedeane G. S. Kenshima, Daniel R. Sousa, Tiago Giorgetti +2

The THz range has been under-explored for solar astronomy, mainly due to technological limitations. Only recently, a few new telescopes, such as the High Altitude Terahertz Solar (…

astro-ph.SR2026

First time delay observation between two mid-infrared channels in solar flare footpoints

Miguel Rojas-Quesada, Lyndsay Fletcher, Hugh Hudson +2

The strong correlation between energy injection and mid-infrared (mid-IR) emission observed during solar flares can be used to probe energy deposition throughout the chromosphere,…

astro-ph.SR2026★ 1 cited

Observational Evidence Linking Loop Length and Thermal-Nonthermal Peak Timing in Solar Flares

S. M. Perriyil, S. S. Sadangaya, C. G. Giménez de Castro +1

We investigate how the magnetic loop length of solar flares relates to the timing between their thermal and nonthermal emission signatures. Our study analyzes a sample of 96 C-, M-…

astro-ph.IM2025

Millimeter-Wavelength Observations of the Active Sun: Unveiling the Origins of Space Weather

Sven Wedemeyer, Stefaan Poedts, Stanislav Gunár +15

Societal dependence on space-based services demands major advances in predicting the impacts of eruptive solar events. Millimeter-wavelength observations offer uniquely direct acce…

astro-ph.SR2024

Precise timing of solar flare footpoint sources from mid-infrared observations

Paulo J. A. Simões, Lyndsay Fletcher, Hugh S. Hudson +3

Solar flares are powerful particle accelerators, and in the accepted standard flare model most of the flare energy is transported from a coronal energy-release region by accelerate…

astro-ph.SR2024★ 4 cited

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Solar and stellar observations

Sven Wedemeyer, Miroslav Barta, Roman Brajsa +35

Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composit…

astro-ph.SR2018★ 29 cited

Solar polar brightening and radius at 100 and 230 GHz observed by ALMA

Caius L. Selhorst, Paulo J. A. Simões, Roman Brajša +8

Polar brightening of the Sun at radio frequencies has been studied for almost fifty years and yet a disagreement persists between solar atmospheric models and observations. Some ob…

astro-ph.SR2014★ 18 cited

Solar Radio Bursts with Spectral Fine Structures in Preflares

Yin Zhang, Baolin Tan, Marian Karlický +4

A good observation of preflare activities is important for us to understand the origin and triggering mechanism of solar flares, and to predict the occurrence of solar flares. This…