Zobrazeno 1 - 10
of 135
pro vyhledávání: '"DEL MORO, DARIO"'
Autor:
Francisco, Grégoire, Ramunno, Francesco Pio, Georgoulis, Manolis K., Fernandes, João, Barata, Teresa, Del Moro, Dario
The solar magnetized corona is responsible for various manifestations with a space weather impact, such as flares, coronal mass ejections (CMEs) and, naturally, the solar wind. Modeling the corona's dynamics and evolution is therefore critical for im
Externí odkaz:
http://arxiv.org/abs/2410.20843
Solar flare forecasting mainly relies on photospheric magnetograms and associated physical features to predict forthcoming flares. However, it is believed that flare initiation mechanisms often originate in the chromosphere and the lower corona. In t
Externí odkaz:
http://arxiv.org/abs/2410.16116
Autor:
Molinaro, Marco, Formato, Valerio, Magnafico, Carmelo, Benvenuto, Federico, Perfetti, Alessandro, De Marco, Rossana, Campi, Cristina, Tacchino, Andrea, di Felice, Valeria, Pietropaolo, Ermanno, de Gasperis, Giancarlo, di Fino, Luca, Francisco, Gregoire, Bertello, Igor, Milillo, Anna, Sindoni, Giuseppe, Plainaki, Christina, Giardino, Marco, Polenta, Gianluca, Del Moro, Dario, Laurenza, Monica
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 prototype of the scientific data centre for Space Weather of the Italian S
Externí odkaz:
http://arxiv.org/abs/2310.16871
Autor:
Stangalini, Marco, Pedichini, Fernando, Pinna, Enrico, Christou, Julian, Hill, John, Puglisi, Alfio, Bailey, Vanessa, Centrone, Mauro, Del Moro, Dario, Esposito, Simone, Fiore, Fabrizio, Giallongo, Emanuele, Hinz, Phil, Vaz, Amali
Residual speckles in adaptive optics (AO) images represent a well-known limitation on the achievement of the contrast needed for faint source detection. Speckles in AO imagery can be the result of either residual atmospheric aberrations, not correcte
Externí odkaz:
http://hdl.handle.net/10150/625223
http://arizona.openrepository.com/arizona/handle/10150/625223
http://arizona.openrepository.com/arizona/handle/10150/625223
Publikováno v:
Advances in Space Research, 2022
Solar flares, along with other sun-originated events such as Coronal Mass Ejections, fast solar wind streams, and solar energetic particles are among the most relevant events in Space Weather. Moreover, solar flares are the most energetic processes t
Externí odkaz:
http://arxiv.org/abs/2211.10189
Autor:
Reda, Raffaele, Giovannelli, Luca, Alberti, Tommaso, Berrilli, Francesco, Bertello, Luca, Del Moro, Dario, Di Mauro, Maria Pia, Giobbi, Piermarco, Penza, Valentina
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023
The Earth's magnetosphere extension is controlled by the solar activity level via solar wind properties. Understanding such a relation in the Solar System is important for predicting also the condition of exoplanetary magnetospheres near Sun-like sta
Externí odkaz:
http://arxiv.org/abs/2203.01554
Autor:
Napoletano, Gianluca, Foldes, Raffaello, Camporeale, Enrico, de Gasperis, Giancarlo, Giovannelli, Luca, Paouris, Evangelos, Pietropaolo, Ermanno, Teunissen, Jannis, Tiwari, Ajay Kumar, Del Moro, Dario
Publikováno v:
Space Weather, 20, e2021SW002925 (2022)
In recent years, ensemble modeling has been widely employed in space weather to estimate uncertainties in forecasts. We here focus on the ensemble modeling of CME arrival times and arrival velocities using a drag-based model, which is well-suited for
Externí odkaz:
http://arxiv.org/abs/2201.12049
Autor:
Cicogna, Domenico, Berrilli, Francesco, Calchetti, Daniele, Del Moro, Dario, Giovannelli, Luca, Benvenuto, Federico, Campi, Cristina, Guastavino, Sabrina, Piana, Michele
Solar flares emanate from solar active regions hosting complex and strong bipolar magnetic fluxes. Estimating the probability of an active region to flare and defining reliable precursors of intense flares is an extremely challenging task in the spac
Externí odkaz:
http://arxiv.org/abs/2105.00897
Autor:
Abbasvand, Vahid, Sobotka, Michal, Heinzel, Petr, Svanda, Michal, Jurcák, Jan, del Moro, Dario, Berrilli, Francesco
Acoustic and magnetoacoustic waves are considered to be possible agents of chromospheric heating. We present a comparison of deposited acoustic energy flux with total integrated radiative losses in the middle chromosphere of the quiet Sun and a weak
Externí odkaz:
http://arxiv.org/abs/2001.03413
Autor:
Keys, Peter H., Reid, Aaron, Mathioudakis, Mihalis, Shelyag, Sergiy, Henriques, Vasco M. J., Hewitt, Rebecca L., Del Moro, Dario, Jafarzadeh, Shahin, Jess, David B., Stangalini, Marco
Publikováno v:
A&A 633, A60 (2020)
Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with field strengths of the order of a kilogauss within intergranular lanes in the photosphere. Aims. Here we study the evolution of various physical proper
Externí odkaz:
http://arxiv.org/abs/1911.08436