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Your search keyword '"Zuccarello, F."' showing total 11 results
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11 results on '"Zuccarello, F."'

1. Understanding the thermal and magnetic properties of a X-class flare in the low solar atmosphere

Author

Ferrente, F., Noda, C. Quintero, Zuccarello, F., and Guglielmino, S. L.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We analyse the spatial distribution and vertical stratification of the physical parameters of the solar atmosphere when an X-class flare occurs. We made use of observations acquired by the Interferometric Bidimensional Spectropolarimeter instrument when observing the full Stokes parameters for the Fe I 6173 A and Ca II 8542 A transitions. We analysed the observed spectra using the newly developed DeSIRe code to infer the atmospheric parameters at photospheric and chromospheric layers over the entire observed field of view. Our findings reveal that the chromosphere is characterised by temperature enhancements and strong upflows in the flare ribbon area, which indicates that the flaring event is producing hot material that is moving outwards from the Sun. We did not detect any trace of temperature enhancements or strong velocities (of any sign) at photospheric layers, signalling that the impact of the flaring event mainly happens at the middle and upper layers. The information about the magnetic field vector revealed relatively smooth stratifications with height for both magnetic field strength and inclination. Still, when examining the spatial distribution of the magnetic field inclination, we observed the presence of large-scale mixed polarities in the regions where the flare ribbon is located. These results suggest that the interaction between those mixed polarities could be the flare's triggering mechanism., Comment: 14 pages, 9 figures

Published
2024
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2. Confinedness of an X3.1 class solar flare occurred in NOAA 12192: Analysis from multi-instruments observations

Author

Vasantharaju, N., Zuccarello, F., Ferrente, F., and Guglielmino, S. L.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

The non-association of coronal mass ejections with high energetic flares is sparse. For this reason, the magnetic conditions required for the confinedness of major flares is a topic of active research. Using multi-instrument observations, we investigated the evolution and effects of confinedness in an X3.1 flare, which occurred in active region (AR) 12192. The decrease of net fluxes in the brightening regions, near the footpoints of the multi-sigmoidal AR in photosphere and chromosphere, indicative of flux cancellation favouring tether-cutting reconnection (TCR), is observed using the magnetic field observations of HMI/SDO and SOT/Hinode, respectively. The analysis of spectropolarimetric data obtained by the Interferometric Bidimensional Spectrometer over the brightening regions suggests untwisting of field lines, which further supports TCR. Filaments near polarity inversion line region, resulted from TCR of low lying sheared loops, undergo merging and form an elongated filament. The temperature and density differences between footpoints of the merged filament, revealed by DEM analysis, caused streaming and counter-streaming of plasma flow along the filament and unloads at its footpoints with an average velocity of $\approx$ 40 km s$^{-1}$. This results in decrease of mass of the filament (density decreased by $>50\%$), leading to its rise and expansion outwards. However, due to strong strapping flux, the filament separates itself instead of erupting. Further, the evolution of non-potential parameters describes the characteristics of confinedness of the flare. Our study suggests that the sigmoid-filament system exhibits upward catastrophe due to mass unloading, but gets suppressed by strong confinement of external poloidal field., Comment: Manuscript has 20 pages, 10 figures and accepted for Publication in the ApJ on 23 April 2023

Published
2023
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3. HiRISE - High-Resolution Imaging and Spectroscopy Explorer - Ultrahigh resolution, interferometric and external occulting coronagraphic science

Author

Erdélyi, Robertus, Damé, Luc, Fludra, Andrzej, Mathioudakis, Mihalis, Amari, T., Belucz, B., Berrilli, F., Bogachev, S., Bolsée, D., Bothmer, V., Brun, S., Dewitte, S., de Wit, T. Dudok, Faurobert, M., Gizon, L., Gyenge, N., Korsós, M. B., Labrosse, N., Matthews, S., Meftah, M., Morgan, H., Pallé, P., Rochus, P., Rozanov, E., Schmieder, B., Tsinganos, K., Verwichte, E., Zharkov, S., Zuccarello, F., and Wimmer-Schweingruber, R.

Published
2022
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7. The CAESAR Project for the ASI Space Weather Infrastructure

Author

Laurenza, M., Moro, D. Del, Alberti, T., Vecchio, A., Zucca, P., Zuccarello, F., Zuccon, P., Laurenza, M., Moro, D. Del, Alberti, T., Vecchio, A., Zucca, P., Zuccarello, F., and Zuccon, P.

Abstract

Contains fulltext : 289942.pdf (Publisher’s version ) (Open Access)

Published
2023

8. The CAESAR Project for the ASI Space Weather Infrastructure

Author

Laurenza, M., primary, Del Moro, D., additional, Alberti, T., additional, Battiston, R., additional, Benella, S., additional, Benvenuto, F., additional, Berrilli, F., additional, Bertello, I., additional, Bertucci, B., additional, Biasiotti, L., additional, Campi, C., additional, Carbone, V., additional, Casolino, M., additional, Cecchi Pestellini, C., additional, Chiappetta, F., additional, Coco, I., additional, Colombo, S., additional, Consolini, G., additional, D’Amicis, R., additional, De Gasperis, G., additional, De Marco, R., additional, Del Corpo, A., additional, Diego, P., additional, Di Felice, V., additional, Di Fino, L., additional, Di Geronimo, C., additional, Faldi, F., additional, Ferrente, F., additional, Feruglio, C., additional, Fiandrini, E., additional, Fiore, F., additional, Foldes, R., additional, Formato, V., additional, Francisco, G., additional, Giannattasio, F., additional, Giardino, M., additional, Giobbi, P., additional, Giovannelli, L., additional, Giusti, M., additional, Gorgi, A., additional, Heilig, B., additional, Iafrate, G., additional, Ivanovski, S. L., additional, Jerse, G., additional, Korsos, M. B., additional, Lepreti, F., additional, Locci, D., additional, Magnafico, C., additional, Mangano, V., additional, Marcucci, M. F., additional, Martucci, M., additional, Massetti, S., additional, Micela, G., additional, Milillo, A., additional, Miteva, R., additional, Molinaro, M., additional, Mugatwala, R., additional, Mura, A., additional, Napoletano, G., additional, Narici, L., additional, Neubüser, C., additional, Nisticò, G., additional, Pauluzzi, M., additional, Perfetti, A., additional, Perri, S., additional, Petralia, A., additional, Pezzopane, M., additional, Piersanti, M., additional, Pietropaolo, E., additional, Pignalberi, A., additional, Plainaki, C., additional, Polenta, G., additional, Primavera, L., additional, Romoli, G., additional, Rossi, M., additional, Santarelli, L., additional, Santi Amantini, G., additional, Siciliano, F., additional, Sindoni, G., additional, Spadoni, S., additional, Sparvoli, R., additional, Stumpo, M., additional, Tomassetti, N., additional, Tozzi, R., additional, Vagelli, V., additional, Vasantharaju, N., additional, Vecchio, A., additional, Vellante, M., additional, Vernetto, S., additional, Vigorito, C., additional, West, M. J., additional, Zimbardo, G., additional, Zucca, P., additional, Zuccarello, F., additional, and Zuccon, P., additional

Published
2023
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9. The European Solar Telescope

Author

Quintero Noda, C., primary, Schlichenmaier, R., additional, Bellot Rubio, L. R., additional, Löfdahl, M. G., additional, Khomenko, E., additional, Jurčák, J., additional, Leenaarts, J., additional, Kuckein, C., additional, González Manrique, S. J., additional, Gunár, S., additional, Nelson, C. J., additional, de la Cruz Rodríguez, J., additional, Tziotziou, K., additional, Tsiropoula, G., additional, Aulanier, G., additional, Aboudarham, J., additional, Allegri, D., additional, Alsina Ballester, E., additional, Amans, J. P., additional, Asensio Ramos, A., additional, Bailén, F. J., additional, Balaguer, M., additional, Baldini, V., additional, Balthasar, H., additional, Barata, T., additional, Barczynski, K., additional, Barreto Cabrera, M., additional, Baur, A., additional, Béchet, C., additional, Beck, C., additional, Belío-Asín, M., additional, Bello-González, N., additional, Belluzzi, L., additional, Bentley, R. D., additional, Berdyugina, S. V., additional, Berghmans, D., additional, Berlicki, A., additional, Berrilli, F., additional, Berkefeld, T., additional, Bettonvil, F., additional, Bianda, M., additional, Bienes Pérez, J., additional, Bonaque-González, S., additional, Brajša, R., additional, Bommier, V., additional, Bourdin, P.-A., additional, Burgos Martín, J., additional, Calchetti, D., additional, Calcines, A., additional, Calvo Tovar, J., additional, Campbell, R. J., additional, Carballo-Martín, Y., additional, Carbone, V., additional, Carlin, E. S., additional, Carlsson, M., additional, Castro López, J., additional, Cavaller, L., additional, Cavallini, F., additional, Cauzzi, G., additional, Cecconi, M., additional, Chulani, H. M., additional, Cirami, R., additional, Consolini, G., additional, Coretti, I., additional, Cosentino, R., additional, Cózar-Castellano, J., additional, Dalmasse, K., additional, Danilovic, S., additional, De Juan Ovelar, M., additional, Del Moro, D., additional, del Pino Alemán, T., additional, del Toro Iniesta, J. C., additional, Denker, C., additional, Dhara, S. K., additional, Di Marcantonio, P., additional, Díaz Baso, C. J., additional, Diercke, A., additional, Dineva, E., additional, Díaz-García, J. J., additional, Doerr, H.-P., additional, Doyle, G., additional, Erdelyi, R., additional, Ermolli, I., additional, Escobar Rodríguez, A., additional, Esteban Pozuelo, S., additional, Faurobert, M., additional, Felipe, T., additional, Feller, A., additional, Feijoo Amoedo, N., additional, Femenía Castellá, B., additional, Fernandes, J., additional, Ferro Rodríguez, I., additional, Figueroa, I., additional, Fletcher, L., additional, Franco Ordovas, A., additional, Gafeira, R., additional, Gardenghi, R., additional, Gelly, B., additional, Giorgi, F., additional, Gisler, D., additional, Giovannelli, L., additional, González, F., additional, González, J. B., additional, González-Cava, J. M., additional, González García, M., additional, Gömöry, P., additional, Gracia, F., additional, Grauf, B., additional, Greco, V., additional, Grivel, C., additional, Guerreiro, N., additional, Guglielmino, S. L., additional, Hammerschlag, R., additional, Hanslmeier, A., additional, Hansteen, V., additional, Heinzel, P., additional, Hernández-Delgado, A., additional, Hernández Suárez, E., additional, Hidalgo, S. L., additional, Hill, F., additional, Hizberger, J., additional, Hofmeister, S., additional, Jägers, A., additional, Janett, G., additional, Jarolim, R., additional, Jess, D., additional, Jiménez Mejías, D., additional, Jolissaint, L., additional, Kamlah, R., additional, Kapitán, J., additional, Kašparová, J., additional, Keller, C. U., additional, Kentischer, T., additional, Kiselman, D., additional, Kleint, L., additional, Klvana, M., additional, Kontogiannis, I., additional, Krishnappa, N., additional, Kučera, A., additional, Labrosse, N., additional, Lagg, A., additional, Landi Degl’Innocenti, E., additional, Langlois, M., additional, Lafon, M., additional, Laforgue, D., additional, Le Men, C., additional, Lepori, B., additional, Lepreti, F., additional, Lindberg, B., additional, Lilje, P. B., additional, López Ariste, A., additional, López Fernández, V. A., additional, López Jiménez, A. C., additional, López López, R., additional, Manso Sainz, R., additional, Marassi, A., additional, Marco de la Rosa, J., additional, Marino, J., additional, Marrero, J., additional, Martín, A., additional, Martín Gálvez, A., additional, Martín Hernando, Y., additional, Masciadri, E., additional, Martínez González, M., additional, Matta-Gómez, A., additional, Mato, A., additional, Mathioudakis, M., additional, Matthews, S., additional, Mein, P., additional, Merlos García, F., additional, Moity, J., additional, Montilla, I., additional, Molinaro, M., additional, Molodij, G., additional, Montoya, L. M., additional, Munari, M., additional, Murabito, M., additional, Núñez Cagigal, M., additional, Oliviero, M., additional, Orozco Suárez, D., additional, Ortiz, A., additional, Padilla-Hernández, C., additional, Paéz Mañá, E., additional, Paletou, F., additional, Pancorbo, J., additional, Pastor Cañedo, A., additional, Pastor Yabar, A., additional, Peat, A. W., additional, Pedichini, F., additional, Peixinho, N., additional, Peñate, J., additional, Pérez de Taoro, A., additional, Peter, H., additional, Petrovay, K., additional, Piazzesi, R., additional, Pietropaolo, E., additional, Pleier, O., additional, Poedts, S., additional, Pötzi, W., additional, Podladchikova, T., additional, Prieto, G., additional, Quintero Nehrkorn, J., additional, Ramelli, R., additional, Ramos Sapena, Y., additional, Rasilla, J. L., additional, Reardon, K., additional, Rebolo, R., additional, Regalado Olivares, S., additional, Reyes García-Talavera, M., additional, Riethmüller, T. L., additional, Rimmele, T., additional, Rodríguez Delgado, H., additional, Rodríguez González, N., additional, Rodríguez-Losada, J. A., additional, Rodríguez Ramos, L. F., additional, Romano, P., additional, Roth, M., additional, Rouppe van der Voort, L., additional, Rudawy, P., additional, Ruiz de Galarreta, C., additional, Rybák, J., additional, Salvade, A., additional, Sánchez-Capuchino, J., additional, Sánchez Rodríguez, M. L., additional, Sangiorgi, M., additional, Sayède, F., additional, Scharmer, G., additional, Scheiffelen, T., additional, Schmidt, W., additional, Schmieder, B., additional, Scirè, C., additional, Scuderi, S., additional, Siegel, B., additional, Sigwarth, M., additional, Simões, P. J. A., additional, Snik, F., additional, Sliepen, G., additional, Sobotka, M., additional, Socas-Navarro, H., additional, Sola La Serna, P., additional, Solanki, S. K., additional, Soler Trujillo, M., additional, Soltau, D., additional, Sordini, A., additional, Sosa Méndez, A., additional, Stangalini, M., additional, Steiner, O., additional, Stenflo, J. O., additional, Štěpán, J., additional, Strassmeier, K. G., additional, Sudar, D., additional, Suematsu, Y., additional, Sütterlin, P., additional, Tallon, M., additional, Temmer, M., additional, Tenegi, F., additional, Tritschler, A., additional, Trujillo Bueno, J., additional, Turchi, A., additional, Utz, D., additional, van Harten, G., additional, van Noort, M., additional, van Werkhoven, T., additional, Vansintjan, R., additional, Vaz Cedillo, J. J., additional, Vega Reyes, N., additional, Verma, M., additional, Veronig, A. M., additional, Viavattene, G., additional, Vitas, N., additional, Vögler, A., additional, von der Lühe, O., additional, Volkmer, R., additional, Waldmann, T. A., additional, Walton, D., additional, Wisniewska, A., additional, Zeman, J., additional, Zeuner, F., additional, Zhang, L. Q., additional, Zuccarello, F., additional, and Collados, M., additional

Published
2022
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10. HiRISE - High-Resolution Imaging and Spectroscopy Explorer - Ultrahigh resolution, interferometric and external occulting coronagraphic science

Author

Erdélyi, R. Damé, L. Fludra, A. Mathioudakis, M. Amari, T. Belucz, B. Berrilli, F. Bogachev, S. Bolsée, D. Bothmer, V. Brun, S. Dewitte, S. de Wit, T.D. Faurobert, M. Gizon, L. Gyenge, N. Korsós, M.B. Labrosse, N. Matthews, S. Meftah, M. Morgan, H. Pallé, P. Rochus, P. Rozanov, E. Schmieder, B. Tsinganos, K. Verwichte, E. Zharkov, S. Zuccarello, F. Wimmer-Schweingruber, R.

Subjects
Physics::Space Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics
Abstract

Recent solar physics missions have shown the definite role of waves and magnetic fields deep in the inner corona, at the chromosphere-corona interface, where dramatic and physically dominant changes occur. HiRISE (High Resolution Imaging and Spectroscopy Explorer), the ambitious new generation ultra-high resolution, interferometric, and coronagraphic, solar physics mission, proposed in response to the ESA Voyage 2050 Call, would address these issues and provide the best-ever and most complete solar observatory, capable of ultra-high spatial, spectral, and temporal resolution observations of the solar atmosphere, from the photosphere to the corona, and of new insights of the solar interior from the core to the photosphere. HiRISE, at the L1 Lagrangian point, would provide meter class FUV imaging and spectro-imaging, EUV and XUV imaging and spectroscopy, magnetic fields measurements, and ambitious and comprehensive coronagraphy by a remote external occulter (two satellites formation flying 375 m apart, with a coronagraph on a chaser satellite). This major and state-of-the-art payload would allow us to characterize temperatures, densities, and velocities in the solar upper chromosphere, transition zone, and inner corona with, in particular, 2D very high resolution multi-spectral imaging-spectroscopy, and, direct coronal magnetic field measurement, thus providing a unique set of tools to understand the structure and onset of coronal heating. HiRISE’s objectives are natural complements to the Parker Solar Probe and Solar Orbiter-type missions. We present the science case for HiRISE which will address: i) the fine structure of the chromosphere-corona interface by 2D spectroscopy in FUV at very high resolution; ii) coronal heating roots in the inner corona by ambitious externally-occulted coronagraphy; iii) resolved and global helioseismology thanks to continuity and stability of observing at the L1 Lagrange point; and iv) solar variability and space climate with, in addition, a global comprehensive view of UV variability. © 2022, The Author(s).

Published
2022

11. Assessing impending hazards from summit eruptions: the new probabilistic map for lava flow inundation at Mt. Etna.

Author

Zuccarello F, Bilotta G, Ganci G, Proietti C, and Cappello A

Abstract

The development of probabilistic maps associated with lava flow inundation is essential to assess hazard in open vent volcanoes, especially those that have highly urbanized flanks. In this study we present the new lava flow hazard map linked to the summit eruptions of Mt. Etna, which has been developed using a probabilistic approach that integrates statistical analyses of the volcanological historical data with numerical simulations of lava flows. The statistical analysis of volcanological data (including vent location, duration and lava volumes) about all summit eruptions occurred since 1998 has allowed us both to estimate the spatiotemporal probability of future vent opening and to extract the effusion rate curves for lava flow modelling. Numerical simulations were run using the GPUFLOW model on a 2022 Digital Surface Model derived from optical satellite images. The probabilistic approach has been validated through a back-analysis by calculating the fit between the expected probabilities of inundation and the lava flows actually emplaced during the 2020-2022 period. The obtained map shows a very high probability of inundation of lava flows emitted at vents linked to the South East Crater, according to the observation of the eruptive dynamics in the last decades., (© 2023. The Author(s).)

Published
2023
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