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Evidence of an upper ionospheric electric field perturbation correlated with a gamma ray burst.
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.
Afiliação
  • Piersanti M; Department of Physical and Chemical Sciences, University of L'Aquila, 67100, L'Aquila, Italy. mirko.piersanti@univaq.it.
  • Ubertini P; National Institute of Astrophysics, IAPS, Rome, 00133, Italy. mirko.piersanti@univaq.it.
  • Battiston R; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Bazzano A; Department of Physics, University of Trento, Povo, Italy.
  • D'Angelo G; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Rodi JG; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Diego P; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Zeren Z; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Ammendola R; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Badoni D; National Institute of Natural Hazards, Ministry of Emergency Management of China, Beijing, 100085, People's Republic of China.
  • Bartocci S; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Beolè S; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Bertello I; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Burger WJ; INFN - Sezione di Torino, 10125, Torino, Italy.
  • Campana D; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Cicone A; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Cipollone P; INFN-Sezione di Napoli, Naples, 80126, Italy.
  • Coli S; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Conti L; Dipartimento di Ingegneria e Scienze dell'Informazione e Matematica, University of L'Aquila, 67100, L'Aquila, Italy.
  • Contin A; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Cristoforetti M; INFN - Sezione di Torino, 10125, Torino, Italy.
  • De Angelis F; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • De Donato C; Uninettuno University, 00186, Rome, Italy.
  • De Santis C; University of Bologna, Bologna, 40127, Italy.
  • Di Luca A; INFN - Sezione di Bologna, 40127, Bologna, Italy.
  • Fiorenza E; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Follega FM; Fondazione Bruno Kessler, 38123, Povo, TN, Italy.
  • Gebbia G; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Iuppa R; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Lega A; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Lolli M; Department of Physics, University of Trento, Povo, Italy.
  • Martino B; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Martucci M; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Masciantonio G; Department of Physics, University of Trento, Povo, Italy.
  • Mergè M; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Mese M; Department of Physics, University of Trento, Povo, Italy.
  • Morbidini A; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Neubüser C; Department of Physics, University of Trento, Povo, Italy.
  • Nozzoli F; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Nuccilli F; Department of Physics, University of Trento, Povo, Italy.
  • Oliva A; TIFPA-INFN, Povo, 38123, Trento, Italy.
  • Osteria G; INFN - Sezione di Bologna, 40127, Bologna, Italy.
  • Palma F; National Institute of Astrophysics, IAPS, Rome, 00133, Italy.
  • Palmonari F; CNR, V. Fosso del Cavaliere 100, 00133, Rome, Italy.
  • Panico B; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Papini E; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Parmentier A; INFN, University of Rome Tor Vergata, Rome, 00133, Italy.
  • Perciballi S; Agenzia Spaziale Italia, Rome, 00133, Italy.
  • Perfetto F; INFN-Sezione di Napoli, Naples, 80126, Italy.
  • Perinelli A; Università degli Studi di Napoli Federico II, 80126, Naples, Italy.
Nat Commun ; 14(1): 7013, 2023 Nov 14.
Article em En | MEDLINE | ID: mdl-37963921
Earth's atmosphere, whose ionization stability plays a fundamental role for the evolution and endurance of life, is exposed to the effect of cosmic explosions producing high energy Gamma-ray-bursts. Being able to abruptly increase the atmospheric ionization, they might deplete stratospheric ozone on a global scale. During the last decades, an average of more than one Gamma-ray-burst per day were recorded. Nevertheless, measurable effects on the ionosphere were rarely observed, in any case on its bottom-side (from about 60 km up to about 350 km of altitude). Here, we report evidence of an intense top-side (about 500 km) ionospheric perturbation induced by significant sudden ionospheric disturbance, and a large variation of the ionospheric electric field at 500 km, which are both correlated with the October 9, 2022 Gamma-ray-burst (GRB221009A).

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article