activity
20112026
most citedThe Relationship Between Solar Radio and Hard X-ray Emission

132 citations · 724 across the 45 of their papers we have counts for

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Showing astro-ph.SRShow all

36 papers · 1 filter

astro-ph.SR2026

Tracking a solar energetic eruption and associated energetic particles from Sun to spacecraft

D. E. Morosan, M. Baumgartner-Steinleitner, K. Bhandari +17

Context. Solar energetic particles (SEPs) in the heliosphere are produced by flaring processes on the Sun or shocks driven by coronal mass ejections (CMEs). Electrons, in particula…

astro-ph.SR2026

Fine-scale downflows above flare ribbons captured by Solar Orbiter/EUI

Zheng Sun, Alexander G. M. Pietrow, Malcolm K. Druett +8

In solar flares, flare ribbons map chromospheric footpoints where flare energy deposition occurs. These locations are associated with field aligned energy transport from the corona…

astro-ph.SR2026

SJET: An Interactive Solar Jet Extraction Tool

Song Tan, Alexander Warmuth, Frédéric Schuller +4

Solar jets are dynamic collimated plasma flows in the solar atmosphere that play crucial roles in coronal heating and solar wind acceleration. Their complex and diverse morphologie…

astro-ph.SR2025

Height-dependent thermal properties of extreme-ultraviolet campfires in the quiet Sun

O. Podladchikova, A. Warmuth, L. Harra +30

Small-scale impulsive energy-release events are widely considered a key ingredient of quiet-Sun coronal heating. We quantified the thermal-energy content of extreme-ultraviolet (EU…

astro-ph.SR2025

Solar Orbiter reveals persistent magnetic reconnection in medium-scale filament eruptions

Song Tan, Alexander Warmuth, Frédéric Schuller +7

Solar filament eruptions play a key role in driving space weather, yet their fine-scale evolution remains poorly understood due to observational limitations. Using unprecedented hi…

astro-ph.SR2025

Extremely diverse coronal jets accompanying an erupting filament captured by Solar Orbiter

Song Tan, Alexander Warmuth, Frédéric Schuller +3

Solar jets are collimated plasma ejections driven by magnetic reconnection, which play a critical role in the energy release and mass transport in the solar atmosphere. Using Solar…

astro-ph.SR2025★ 6 cited

CoSEE-Cat: A Comprehensive Solar Energetic Electron event Catalogue obtained from combined in situ and remote-sensing observations from Solar Orbiter -- Catalogue description and first statistical results

A. Warmuth, F. Schuller, R. Gómez-Herrero +39

(abridged) The acceleration of particles at the Sun and their propagation through interplanetary space are key topics in heliophysics. Specifically, solar energetic electrons (SEEs…

astro-ph.SR2025

Ion acceleration in Fermi-LAT behind-the-limb solar flares: the role of coronal shock waves

Alexander Warmuth, Melissa Pesce-Rollins, Nicola Omodei +1

We investigate the relationship between the gamma-ray emission measured with Fermi-LAT and radio signatures of coronal shock waves in four behind-the-limb (BTL) solar flares. All e…

astro-ph.SR2025★ 11 cited

On the reason for the widespread energetic storm particle event of 13 March 2023

N. Dresing, I. C. Jebaraj, N. Wijsen +20

On 13 March 2023, when the Parker Solar Probe was situated on the far side of the Sun as seen from Earth, a large solar eruption took place creating a strong solar energetic partic…

astro-ph.SR2024★ 4 cited

Determining the acceleration regions of in situ electrons using remote radio and X-ray observations

D. E. Morosan, N. Dresing, C. Palmroos +13

Solar energetic particles in the heliosphere are produced by flaring processes on the Sun or shocks driven by coronal mass ejections. These particles are regularly detected remotel…

astro-ph.SR2024★ 14 cited

Solar energetic particles injected inside and outside a magnetic cloud: The widespread solar energetic particle event on 2022 January 20

L. Rodríguez-García, R. Gómez-Herrero, N. Dresing +22

Context. On 2022 January 20, the Energetic Particle Detector (EPD) on board Solar Orbiter measured a solar energetic particle (SEP) event showing unusual first arriving particles f…

astro-ph.SR2024★ 5 cited

Temperature and differential emission measure evolution of a limb flare on 13 January 2015

Malte Bröse, Alexander Warmuth, Taro Sakao +1

Spatially unresolved observations show that the cooling phase in solar flares can be much longer than theoretical models predict. It has not yet been determined whether this is als…

astro-ph.SR2023★ 25 cited

The existence of hot X-ray onsets in solar flares

Andrea Francesco Battaglia, Hugh Hudson, Alexander Warmuth +9

It is well known among the scientific community that solar flare activity often begins well before the main impulsive energy release. Our aim is to investigate the earliest phase o…

astro-ph.SR2023★ 17 cited

A multiple spacecraft detection of the 2 April 2022 M-class flare and filament eruption during the first close Solar Orbiter perihelion

M. Janvier, S. Mzerguat, P. R. Young +56

The Solar Orbiter mission completed its first remote-sensing observation windows in the spring of 2022. On 2/4/2022, an M-class flare followed by a filament eruption was seen both…

astro-ph.SR2023

Observational signatures of electron-driven chromospheric evaporation in a white-light flare

Dong Li, Chuan Li, Ye Qiu +7

We investigate observational signatures of explosive chromospheric evaporation during a white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis, bisector…

astro-ph.SR2023★ 6 cited

Global energetics of solar powerful events on 6 September 2017

Dong Li, Alexander Warmuth, Jincheng Wang +9

Solar flares and coronal mass ejections (CMEs) are thought to be the most powerful events on the Sun. They can release energy as high as 10^32 erg in tens of minutes,and could prod…

astro-ph.SR2023★ 50 cited

The 17 April 2021 widespread solar energetic particle event

N. Dresing, L. Rodríguez-García, I. C. Jebaraj +46

Context. A solar eruption on 17 April 2021 produced a widespread Solar Energetic Particle (SEP) event that was observed by five longitudinally well-separated observers in the inner…

astro-ph.SR2023★ 3 cited

Parametric study of the kinematic evolution of coronal mass ejection shock waves and their relation to flaring activity

Manon Jarry, Alexis P. Rouillard, Illya Plotnikov +2

Coronal and interplanetary shock waves produced by coronal mass ejections (CMEs) are major drivers of space-weather phenomena, inducing major changes in the heliospheric radiation…

astro-ph.SR2023★ 6 cited

Multi-point study of the energy release and impulsive CME dynamics in an eruptive C7 flare

J. Saqri, A. M. Veronig, E. C. M. Dickson +6

We combine observations from different vantage points to perform a detailed study of a long duration eruptive C7 class flare that occurred on 17 April 2021 and was partially occult…

astro-ph.SR2023★ 42 cited

The data center for the Spectrometer and Telescope for Imaging X-rays (STIX) onboard Solar Orbiter

Hualin Xiao, Shane Maloney, Säm Krucker +12

The Spectrometer and Telescope for Imaging X-rays (STIX) on board Solar Orbiter observes solar X-ray emission in the range of 4 – 150 keV and produces spectra and images of s…

astro-ph.SR2023★ 27 cited

Multiple injections of energetic electrons associated with the flare/CME event on 9 October 2021

Immanuel Christopher Jebaraj, Athanasios Kouloumvakos, Nina Dresing +11

We study the solar energetic particle (SEP) event observed on 9 October 2021, by multiple spacecraft including Solar Orbiter (SolO). The event was associated with an M1.6 flare, a…

astro-ph.SR2022★ 14 cited

Identifying the energy release site in a Solar microflare with a jet

Andrea Francesco Battaglia, Wen Wang, Jonas Saqri +10

One of the main science questions of the Solar Orbiter and Parker Solar Probe missions deals with understanding how electrons in the lower solar corona are accelerated and how they…

astro-ph.SR2022★ 6 cited

Interferometric imaging of the type IIIb and U radio bursts observed with LOFAR on 22 August 2017

Bartosz Dabrowski, Katarzyna Mikula, Pawel Flisek +18

The Sun is the source of different types of radio bursts that are associated with solar flares, for example. Among the most frequently observed phenomena are type III solar bursts.…

astro-ph.SR2022★ 18 cited

The coupling of an EUV coronal wave and ion acceleration in a Fermi-LAT behind-the-limb solar flare

Melissa Pesce-Rollins, Nicola Omodei, Sam Krucker +6

We present the Fermi-LAT observations of the behind-the-limb (BTL) flare of July 17, 2021 and the joint detection of this flare by STIX onboard Solar Orbiter. The separation betwee…