output
20042026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations

Showing 2022 · astro-ph.SRShow all

16 papers · 2 filters

astro-ph.SR2022★ 24 cited

Solar flare hard X-rays from the anchor points of an eruptive filament

Muriel Zoë Stiefel, Andrea Francesco Battaglia, Krzysztof Barczynski +7

Context. We present an analysis of a GOES M1.8 flare with excellent observational coverage in UV, EUV, and X-ray, including observations from the instruments IRIS, SDO with AIA, Hi…

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★ 8 cited

Flares detected in ALMA single-dish images of the Sun

I. Skokić, A. O. Benz, R. Brajša +3

The (sub)millimeter radiation of solar flares is poorly understood. Without spatial resolution, it cannot be compared easily to flare emissions in other wavelengths. The Atacama La…

astro-ph.SR2022★ 9 cited

Multiple Regions of Nonthermal Quasi-Periodic Pulsations during the Impulsive Phase of a Solar Flare

Yingjie Luo, Bin Chen, Sijie Yu +2

Flare-associated quasiperiodic pulsations (QPPs) in radio and X-ray wavelengths, particularly those related to nonthermal electrons, contain important information about the energy…

astro-ph.SR2022★ 12 cited

The First Survey of Quiet Sun Features Observed in Hard X-Rays With NuSTAR

Sarah Paterson, Iain G. Hannah, Brian W. Grefenstette +5

We present the first survey of quiet Sun features observed in hard X-rays (HXRs), using the the Nuclear Spectroscopic Telescope ARray (NuSTAR), a HXR focusing optics telescope. The…

astro-ph.SR2022★ 13 cited

Detection of weak ubiquitous impulsive nonthermal emissions from the solar corona

Rohit Sharma, Divya Oberoi, Marina Battaglia +1

A ubiquitous presence of weak energy releases is one of the most promising hypotheses to explain coronal heating, referred to as the nanoflare hypothesis. The accelerated electrons…

astro-ph.SR2022★ 5 cited

The Lyman- Emission in a C1.4 Solar Flare Observed by the Extreme Ultraviolet Imager aboard Solar Orbiter

Ying Li, Qiao Li, De-Chao Song +7

The hydrogen Lyman- (H {\sc i} Ly) emission during solar flares has rarely been studied in spatially resolved images and its physical origin has not been fully understood. In…

astro-ph.SR2022★ 4 cited

Observations of Thomson scattering from a loop-prominence system

Juan Carlos Martínez Oliveros, Juan Camilo Guevara Gómez, Pascal Saint-Hilaire +2

We describe observations of the white-light structures in the low corona following the X8.2 flare SOL2017-09-10, as observed in full Stokes parameters by the Helioseismic and Magne…

astro-ph.SR2022★ 5 cited

Spatial distribution of jets in solar active regions

Jonas Odermatt, Krzysztof Barczynski, Louise K. Harra +2

Context. Solar active regions are known to have jets. These jets are associated with heating and the release of particles into the solar wind. Aim. Our aim is to understand the spa…

astro-ph.SR2022★ 3 cited

The Spectrometer Telescope for Imaging X-rays (STIX) on Solar Orbiter

Laura A. Hayes, Sophie Musset, Daniel M üller +1

The Spectrometer/Telescope for Imaging X-rays (STIX) is one of the 10 instruments on-board the scientific payload of ESA's Solar Orbiter mission. STIX provides hard X-ray imaging s…

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…

astro-ph.SR2022★ 9 cited

On the faintest solar coronal hard X-rays observed with FOXSI

Juan Camilo Buitrago-Casas, Lindsay Glesener, Steven Christe +23

Solar nanoflares are small eruptive events releasing magnetic energy in the quiet corona. If nanoflares follow the same physics as their larger counterparts, they should emit hard…

astro-ph.SR2022★ 28 cited

Forward-fitting STIX visibilities

Anna Volpara, Paolo Massa, Emma Perracchione +6

Aima. To determine to what extent the problem of forward fitting visibilities measured by the Spectrometer/Telescope Imaging X-rays (STIX) on-board Solar Orbiter is more challengin…

astro-ph.SR2022★ 7 cited

Using Multiple Instance Learning for Explainable Solar Flare Prediction

Cédric Huwyler, Martin Melchior

In this work we leverage a weakly-labeled dataset of spectral data from NASAs IRIS satellite for the prediction of solar flares using the Multiple Instance Learning (MIL) paradigm.…

astro-ph.SR2022

First hard X-ray imaging results by Solar Orbiter STIX

Paolo Massa, Andrea F. Battaglia, Anna Volpara +15

Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is one of 6 remote sensing instruments on-board Solar Orbiter. It provides hard X-ray imaging spectroscopy of solar fl…

astro-ph.SR2022★ 15 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…