no code implementations • 14 Mar 2024 • Sabrina Guastavino, Katsiaryna Bahamazava, Emma Perracchione, Fabiana Camattari, Gianluca Audone, Daniele Telloni, Roberto Susino, Gianalfredo Nicolini, Silvano Fineschi, Michele Piana, Anna Maria Massone
This study addresses the prediction of geomagnetic disturbances by exploiting machine learning techniques.
no code implementations • 2 Jan 2024 • Michele Piana, Federico Benvenuto, Anna Maria Massone, Cristina Campi, Sabrina Guastavino, Francesco Marchetti, Paolo Massa, Emma Perracchione, Anna Volpara
AI-FLARES (Artificial Intelligence for the Analysis of Solar Flares Data) is a research project funded by the Agenzia Spaziale Italiana and by the Istituto Nazionale di Astrofisica within the framework of the ``Attivit\`a di Studio per la Comunit\`a Scientifica Nazionale Sole, Sistema Solare ed Esopianeti'' program.
no code implementations • 17 May 2023 • Sabrina Guastavino, Valentina Candiani, Alessandro Bemporad, Francesco Marchetti, Federico Benvenuto, Anna Maria Massone, Roberto Susino, Daniele Telloni, Silvano Fineschi, Michele Piana
Coronal Mass Ejections (CMEs) correspond to dramatic expulsions of plasma and magnetic field from the solar corona into the heliosphere.
no code implementations • 27 Dec 2020 • Emma Perracchione, Paolo Massa, Anna Maria Massone, Michele Piana
Space telescopes for solar hard X-ray imaging provide observations made of sampled Fourier components of the incoming photon flux.
no code implementations • 5 Jul 2020 • Federico Benvenuto, Cristina Campi, Anna Maria Massone, Michele Piana
Machine learning is nowadays the methodology of choice for flare forecasting and supervised techniques, in both their traditional and deep versions, are becoming the most frequently used ones for prediction in this area of space weather.
no code implementations • 18 Feb 2020 • Paolo Massa, Richard Schwartz, A Kim Tolbert, Anna Maria Massone, Brian R Dennis, Michele Piana, Federico Benvenuto
Although widely used in image deconvolution, this method has been formulated in radio astronomy for the analysis of observations in the spatial frequency domain, and an Interactive Data Language (IDL) code has been implemented for image reconstruction from solar X-ray Fourier data.
Image Deconvolution Image Reconstruction +1 Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics 49N45, 94A08
no code implementations • 24 Jan 2020 • Daniela Schenonea, Rita Lai, Michele Cea, Federica Rossi, Lorenzo Torri, Bianca Bignotti, Giulia Succio, Stefano Gualco, Alessio Conte, Alida Dominietto, Anna Maria Massone, Michele Piana, Cristina Campi, Francesco Frassoni, Gianmario Sambuceti, Alberto Stefano Tagliafico
Multiple Myeloma (MM) is a blood cancer implying bone marrow involvement, renal damages and osteolytic lesions.
no code implementations • 8 Apr 2019 • Sabrina Guastavino, Michele Piana, Anna Maria Massone, Richard Schwartz, Federico Benvenuto
Image saturation has been an issue for several instruments in solar astronomy, mainly at EUV wavelengths.
no code implementations • 4 Apr 2019 • Mauro C. Beltrametti, Cristina Campi, Anna Maria Massone, Maria-Laura Torrente
In the framework of the Hough transform technique to detect curves in images, we provide a bound for the number of Hough transforms to be considered for a successful optimization of the accumulator function in the recognition algorithm.
no code implementations • 21 Jun 2017 • Federico Benvenuto, Michele Piana, Cristina Campi, Anna Maria Massone
We introduce a hybrid approach to solar flare prediction, whereby a supervised regularization method is used to realize feature importance and an unsupervised clustering method is used to realize the binary flare/no-flare decision.
no code implementations • 8 Mar 2015 • Richard A Schwartz, Gabriele Torre, Anna Maria Massone, Michele Piana
Saturation affects a significant rate of images recorded by the Atmospheric Imaging Assembly on the Solar Dynamics Observatory.
no code implementations • 15 Jul 2014 • Giorgio Ricca, Mauro C. Beltrametti, Anna Maria Massone
Many bone shapes in the human skeleton are characterized by profiles that can be associated to equations of algebraic curves.