output
19972026
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 2024Show all

10 papers · 1 filter

astro-ph.SR2024★ 1 cited

SPACE-SUIT: An Artificial Intelligence Based Chromospheric Feature Extractor and Classifier for SUIT

Pranava Seth, Vishal Upendran, Megha Anand +6

The Solar Ultraviolet Imaging Telescope(SUIT) onboard Aditya-L1 is an imager that observes the solar photosphere and chromosphere through observations in the wavelength range of 20…

astro-ph.SR2024★ 1 cited

Detection asymmetry in solar energetic particle events

S. Dalla, A. Hutchinson, R. A. Hyndman +6

Context. Solar energetic particles (SEPs) are detected in interplanetary space in association with solar flares and coronal mass ejections (CMEs). The magnetic connection between t…

astro-ph.SR2024★ 5 cited

Magnetic diffusion in Solar atmosphere produces measurable electric fields

Tetsu Anan, Roberto Casini, Han Uitenbroek +13

The efficient release of magnetic energy in astrophysical plasmas, such as during solar flares, can in principle be achieved through magnetic diffusion, at a rate determined by the…

astro-ph.SR2024★ 2 cited

On Thermal Conduction in the Solar Atmosphere: An Analytical Solution for Nonlinear Diffusivity without Compact Support

Sondre Vik Furuseth, George Cherry, Juan Martínez-Sykora

The scientific community employs complicated multiphysics simulations to understand the physics in Solar, Stellar, and Interstellar media. These must be tested against known soluti…

quant-ph2024★ 2 cited

Benchmarking the performance of a high-Q cavity qudit using random unitaries

Nicholas Bornman, Tanay Roy, Joshua A. Job +4

High-coherence cavity resonators are excellent resources for encoding quantum information in higher-dimensional Hilbert spaces, moving beyond traditional qubit-based platforms. A n…

astro-ph.EP2024★ 41 cited

A Contact Binary Satellite of the Asteroid (152830) Dinkinesh

Harold F. Levison, Simone Marchi, Keith S. Noll +3

Asteroids with diameters less than about 5 km have complex histories because they are small enough for radiative torques, YORP, to be a notable factor in their evolution. (152830)…

astro-ph.HE2024★ 9 cited

Mixing of hot shocked plasma with cold gas in Nova YZ Ret 2020

Sharon Mitrani, Ehud Behar, Jeremy J. Drake +5

The origin of bright X-ray emission lines that appear late in a nova eruption remains largely a puzzle. We present two high-resolution X-ray grating spectra of the classical nova Y…

astro-ph.SR2024★ 6 cited

Extreme-ultraviolet (EUV) observables of simulated plasmoid-mediated reconnection in the solar corona

Ø. H. Færder, D. Nóbrega-Siverio, M. Carlsson +1

Understanding the role of magnetic reconnection in the heating and dynamics of the solar atmosphere requires detailed observational data of any observable aspect of the reconnectio…

astro-ph.SR2024★ 11 cited

Small-scale magnetic flux emergence preceding a chain of energetic solar atmospheric events

D. Nóbrega-Siverio, I. Cabello, S. Bose +4

Advancements in instrumentation have revealed a multitude of small-scale EUV events in the solar atmosphere. Our aim is to employ high-resolution magnetograms to gain a detailed un…

astro-ph.SR2024★ 27 cited

Localising pulsations in the hard X-ray and microwave emission of an X-class flare

Hannah Collier, Laura A. Hayes, Sijie Yu +5

Aims: This work aims to identify the mechanism driving pulsations in hard X-ray (HXR) and microwave emission during solar flares. Here, by using combined HXR and microwave observat…