activity
20122025
most citedForecasting Solar Flares Using Magnetogram-based Predictors and Machine Learning

177 citations · 661 across the 41 of their papers we have counts for

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Showing astro-ph.IMShow all

6 papers · 1 filter

astro-ph.IM2023

CAESAR: Space Weather archive prototype for ASPIS

Marco Molinaro, Valerio Formato, Carmelo Magnafico +18

The project CAESAR (Comprehensive spAce wEather Studies for the ASPIS prototype Realization) is aimed to tackle all the relevant aspects of Space Weather (SWE) and realize the prot…

astro-ph.IM2023

STIX imaging I -- Concept

Paolo Massa, Gordon. J. Hurford, Anna Volpara +17

Aims. To provide a schematic mathematical description of the imaging concept of the Spectrometer/Telescope for Imaging X-rays (STIX) on board Solar Orbiter. The derived model is th…

astro-ph.IM2019★ 30 cited

A count-based imaging model for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter

Paolo Massa, Michele Piana, Anna Maria Massone +1

The Spectrometer/Telescope for Imaging X-rays (STIX) will look at solar flares across the hard X-ray window provided by the Solar Orbiter cluster. Similarly to the Reuven Ramaty Hi…

astro-ph.IM2018★ 1 cited

FLARECAST: an I4.0 technology for space weather using satellite data

Michele Piana, Anna Maria Massone, Federico Benvenuto +1

'Flare Likelihood and Region Eruption Forecasting (FLARECAST)' is a Horizon 2020 project, which realized a technological platform for machine learning algorithms, with the objectiv…

astro-ph.IM2015★ 11 cited

Inverse diffraction for the Atmospheric Imaging Assembly in the Solar Dynamics Observatory

Gabriele Torre, Richard A Schwartz, Federico Benvenuto +2

The Atmospheric Imaging Assembly in the Solar Dynamics Observatory provides full Sun images every 1 seconds in each of 7 Extreme Ultraviolet passbands. However, for a significant a…

astro-ph.IM2013★ 31 cited

Expectation Maximization for Hard X-ray Count Modulation Profiles

Federico Benvenuto, Richard Schwartz, Michele Piana +1

This paper is concerned with the image reconstruction problem when the measured data are solar hard X-ray modulation profiles obtained from the Reuven Ramaty High Energy Solar Spec…