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19 results on '"Bertello, Igor"'

1. CAESAR: Space Weather archive prototype for ASPIS

Author

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, and Laurenza, Monica

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

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 Space Agency (ASI) called ASPIS (ASI SPace Weather InfraStructure). This contribution is meant to bring attention upon the first steps in the development of the CAESAR prototype for ASPIS and will focus on the activities of the Node 2000 of CAESAR, the set of Work Packages dedicated to the technical design and implementation of the CAESAR ASPIS archive prototype. The product specifications of the intended resources that will form the archive, functional and system requirements gathered as first steps to seed the design of the prototype infrastructure, and evaluation of existing frameworks, tools and standards, will be presented as well as the status of the project in its initial stage., Comment: 4 pages, 2 figures, ADASS XXXII (2022) Proceedings

Published
2023

2. Gamma-Ray Burst observations by the high-energy charged particle detector on board the CSES-01 satellite between 2019 and 2021

Author

Palma, Francesco, Martucci, Matteo, Neubüser, Coralie, Sotgiu, Alessandro, Follega, Francesco Maria, Ubertini, Pietro, Bazzano, Angela, Rodi, James, Ammendola, Roberto, Badoni, Davide, Bartocci, Simona, Battiston, Roberto, Beolè, Stefania, Bertello, Igor, Burger, William Jerome, Campana, Donatella, Cicone, Antonio, Cipollone, Piero, Coli, Silvia, Conti, Livio, Contin, Andrea, Cristoforetti, Marco, D'Angelo, Giulia, De Angelis, Fabrizio, De Donato, Cinzia, De Santis, Cristian, Diego, Piero, Di Luca, Andrea, Fiorenza, Emiliano, Gebbia, Giuseppe, Iuppa, Roberto, Lega, Alessandro, Lolli, Mauro, Martino, Bruno, Masciantonio, Giuseppe, Mergè, Matteo, Mese, Marco, Morbidini, Alfredo, Nozzoli, Francesco, Nuccilli, Fabrizio, Oliva, Alberto, Osteria, Giuseppe, Palmonari, Federico, Panico, Beatrice, Papini, Emanuele, Parmentier, Alexandra, Perciballi, Stefania, Perfetto, Francesco, Perinelli, Alessio, Picozza, Piergiorgio, Piersanti, Mirko, Pozzato, Michele, Rebustini, Gianmaria, Recchiuti, Dario, Ricci, Ester, Ricci, Marco, Ricciarini, Sergio Bruno, Russi, Andrea, Sahnoun, Zouleikha, Savino, Umberto, Scotti, Valentina, Shen, Xuhui, Sparvoli, Roberta, Tofani, Silvia, Vertolli, Nello, Vilona, Veronica, Vitale, Vincenzo, Zannoni, Ugo, Zeren, Zhima, Zoffoli, Simona, and Zuccon, Paolo

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

In this paper we report the detection of five strong Gamma-Ray Bursts (GRBs) by the High-Energy Particle Detector (HEPD-01) mounted on board the China Seismo-Electromagnetic Satellite (CSES-01), operational since 2018 on a Sun-synchronous polar orbit at a $\sim$ 507 km altitude and 97$^\circ$ inclination. HEPD-01 was designed to detect high-energy electrons in the energy range 3 - 100 MeV, protons in the range 30 - 300 MeV, and light nuclei in the range 30 - 300 MeV/n. Nonetheless, Monte Carlo simulations have shown HEPD-01 is sensitive to gamma-ray photons in the energy range 300 keV - 50 MeV, even if with a moderate effective area above $\sim$ 5 MeV. A dedicated time correlation analysis between GRBs reported in literature and signals from a set of HEPD-01 trigger configuration masks has confirmed the anticipated detector sensitivity to high-energy photons. A comparison between the simultaneous time profiles of HEPD-01 electron fluxes and photons from GRB190114C, GRB190305A, GRB190928A, GRB200826B and GRB211211A has shown a remarkable similarity, in spite of the different energy ranges. The high-energy response, with peak sensitivity at about 2 MeV, and moderate effective area of the detector in the actual flight configuration explain why these five GRBs, characterised by a fluence above $\sim$ 3 $\times$ 10$^{-5}$ erg cm$^{-2}$ in the energy interval 300 keV - 50 MeV, have been detected., Comment: Accepted for publication in The Astrophysical Journal (ApJ)

Published
2023

3. Author Correction: Evidence of an upper ionospheric electric field perturbation correlated with a gamma ray burst

Author

Piersanti, Mirko, Ubertini, Pietro, Battiston, Roberto, Bazzano, Angela, D’Angelo, Giulia, Rodi, James G., Diego, Piero, Zeren, Zhima, Ammendola, Roberto, Badoni, Davide, Bartocci, Simona, Beolè, Stefania, Bertello, Igor, Burger, William J., Campana, Donatella, Cicone, Antonio, Cipollone, Piero, Coli, Silvia, Conti, Livio, Contin, Andrea, Cristoforetti, Marco, De Angelis, Fabrizio, De Donato, Cinzia, De Santis, Cristian, Di Luca, Andrea, Fiorenza, Emiliano, Follega, Francesco Maria, Gebbia, Giuseppe, Iuppa, Roberto, Lega, Alessandro, Lolli, Mauro, Martino, Bruno, Martucci, Matteo, Masciantonio, Giuseppe, Mergè, Matteo, Mese, Marco, Morbidini, Alfredo, Neubüser, Coralie, Nozzoli, Francesco, Nuccilli, Fabrizio, Oliva, Alberto, Osteria, Giuseppe, Palma, Francesco, Palmonari, Federico, Panico, Beatrice, Papini, Emanuele, Parmentier, Alexandra, Perciballi, Stefania, Perfetto, Francesco, Perinelli, Alessio, Picozza, Piergiorgio, Pozzato, Michele, Rebustini, Gianmaria, Recchiuti, Dario, Ricci, Ester, Ricci, Marco, Ricciarini, Sergio B., Russi, Andrea, Sahnoun, Zuleika, Savino, Umberto, Scotti, Valentina, Shen, Xuhui, Sotgiu, Alessandro, Sparvoli, Roberta, Tofani, Silvia, Vertolli, Nello, Vilona, Veronica, Vitale, Vincenzo, Zannoni, Ugo, Zoffoli, Simona, and Zuccon, Paolo

Published
2023
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4. Evidence of an upper ionospheric electric field perturbation correlated with a gamma ray burst

Author

Piersanti, Mirko, Ubertini, Pietro, Battiston, Roberto, Bazzano, Angela, D’Angelo, Giulia, Rodi, James G., Diego, Piero, Zeren, Zhima, Ammendola, Roberto, Badoni, Davide, Bartocci, Simona, Beolè, Stefania, Bertello, Igor, Burger, William J., Campana, Donatella, Cicone, Antonio, Cipollone, Piero, Coli, Silvia, Conti, Livio, Contin, Andrea, Cristoforetti, Marco, De Angelis, Fabrizio, De Donato, Cinzia, De Santis, Cristian, Di Luca, Andrea, Fiorenza, Emiliano, Follega, Francesco Maria, Gebbia, Giuseppe, Iuppa, Roberto, Lega, Alessandro, Lolli, Mauro, Martino, Bruno, Martucci, Matteo, Masciantonio, Giuseppe, Mergè, Matteo, Mese, Marco, Morbidini, Alfredo, Neubüser, Coralie, Nozzoli, Francesco, Nuccilli, Fabrizio, Oliva, Alberto, Osteria, Giuseppe, Palma, Francesco, Palmonari, Federico, Panico, Beatrice, Papini, Emanuele, Parmentier, Alexandra, Perciballi, Stefania, Perfetto, Francesco, Perinelli, Alessio, Picozza, Piergiorgio, Pozzato, Michele, Rebustini, Gianmaria, Recchiuti, Dario, Ricci, Ester, Ricci, Marco, Ricciarini, Sergio B., Russi, Andrea, Sahnoun, Zuleika, Savino, Umberto, Scotti, Valentina, Shen, Xuhui, Sotgiu, Alessandro, Sparvoli, Roberta, Tofani, Silvia, Vertolli, Nello, Vilona, Veronica, Vitale, Vincenzo, Zannoni, Ugo, Zoffoli, Simona, and Zuccon, Paolo

Published
2023
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6. Statistical validation of the Magnetospheric–Ionospheric–Lithospheric Coupling model on occasion of the Marche Earthquake (Mw 4.2) main shock occurred on November 20th 2022

Author

Piersanti, Mirko, primary, D'Angelo, Giulia, additional, Battiston, Roberto, additional, Bertello, Igor, additional, Cicone, Antonio, additional, Diego, Piero, additional, Papini, Emanuele, additional, Parmentier, Alexandra, additional, Recchiuti, Dario, additional, and Ubertini, Pietro, additional

Published
2023
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7. Haiti Earthquake (Mw 7.2): Magnetospheric–Ionospheric–Lithospheric Coupling during and after the Main Shock on 14 August 2021

Author

D’Angelo, Giulia, primary, Piersanti, Mirko, additional, Battiston, Roberto, additional, Bertello, Igor, additional, Carbone, Vincenzo, additional, Cicone, Antonio, additional, Diego, Piero, additional, Papini, Emanuele, additional, Parmentier, Alexandra, additional, Picozza, Piergiorgio, additional, Plainaki, Christina, additional, Recchiuti, Dario, additional, Sparvoli, Roberta, additional, and Ubertini, Pietro, additional

Published
2022
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8. Investigation of the Magnetospheric–Ionospheric–Lithospheric Coupling on occasion of the 14 August 2021 Haitian Earthquake

Author

D'Angelo, Giulia, primary, Piersanti, Mirko, additional, Battiston, Roberto, additional, Bertello, Igor, additional, Cicone, Antonio, additional, Diego, Piero, additional, Follega, Francesco, additional, Iuppa, Roberto, additional, Neubuser, Coralie, additional, Papini, Emanuele, additional, Parmentier, Alexandra, additional, Recchiuti, Dario, additional, and Ubertini, Pietro, additional

Published
2022
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9. Haiti Earthquake (Mw 7.2): Magnetospheric–Ionospheric–Lithospheric Coupling during and after the Main Shock on 14 August 2021.

Author

D'Angelo, Giulia, Piersanti, Mirko, Battiston, Roberto, Bertello, Igor, Carbone, Vincenzo, Cicone, Antonio, Diego, Piero, Papini, Emanuele, Parmentier, Alexandra, Picozza, Piergiorgio, Plainaki, Christina, Recchiuti, Dario, Sparvoli, Roberta, and Ubertini, Pietro

Subjects
IONOSPHERIC plasma, GRAVITY waves, ATMOSPHERIC temperature, PLASMA density, ATMOSPHERIC waves, EARTHQUAKES, EARTHQUAKE aftershocks, SOLAR atmosphere
Abstract

In the last few decades, the efforts of the scientific community to search earthquake signatures in the atmospheric, ionospheric and magnetospheric media have grown rapidly. The increasing amount of good quality data from both ground stations and satellites has allowed for the detections of anomalies with high statistical significance such as ionospheric plasma density perturbations and/or atmospheric temperature and pressure changes. However, the identification of a causal link between the observed anomalies and their possible seismic trigger has so far been prevented by difficulties in the identification of confounders (such as solar and atmospheric activity) and the lack of a global analytical lithospheric–atmospheric–magnetospheric model able to explain (and possibly forecast) any anomalous signal. In order to overcome these problems, we have performed a multi-instrument analysis of a low-latitude seismic event by using high-quality data from both ground bases and satellites and preserving their statistical significance. An earthquake (Mw = 7.2) occurred in the Caribbean region on 14 August 2021 under both solar quiet and fair weather conditions, thus proving an optimal case study to reconstruct the link between the lithosphere, atmosphere, ionosphere, and magnetosphere. The good match between the observations and novel magnetospheric–ionospheric–lithospheric coupling (M.I.L.C.) modeling of the event confirmed that the fault break generated an atmospheric gravity wave that was able to mechanically perturb the ionospheric plasma density, in turn triggering a variation in the magnetospheric field line resonance frequency. [ABSTRACT FROM AUTHOR]

Published
2022
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10. The Electric Field Detector on Board the China Seismo Electromagnetic Satellite—In-Orbit Results and Validation

Author

Diego, Piero, primary, Huang, Jianping, additional, Piersanti, Mirko, additional, Badoni, Davide, additional, Zeren, Zhima, additional, Yan, Rui, additional, Rebustini, Gianmaria, additional, Ammendola, Roberto, additional, Candidi, Maurizio, additional, Guan, Yi-Bing, additional, Lei, Jungang, additional, Masciantonio, Giuseppe, additional, Bertello, Igor, additional, De Santis, Cristian, additional, Ubertini, Pietro, additional, Shen, Xuhui, additional, and Picozza, Piergiorgio, additional

Published
2020
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15. Discrimination between Internal and External origin contributions from LEO satellite magnetic field data.

Author

Bertello, Igor, Cicone, Antonio, Consolini, Giuseppe, Materassi, Massimo, Diego, Piero, Piersanti, Mirko, and Ubertini, Pietro

Subjects
*MAGNETIC fields, *GEOMAGNETISM, *SPACE environment, *ORBITS of artificial satellites, *ARTIFICIAL satellites, *STATISTICS, *MAGNETOPAUSE
Abstract

The evaluation of the external origin contribution (B_EXT) in geomagnetic field satellite observations in the near Earth location (1.2 R_E

Published
2019

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