Nature Communications (Nov 2023)
Evidence of an upper ionospheric electric field perturbation correlated with a gamma ray burst
- Mirko Piersanti,
- Pietro Ubertini,
- Roberto Battiston,
- Angela Bazzano,
- Giulia D’Angelo,
- James G. Rodi,
- Piero Diego,
- Zhima Zeren,
- Roberto Ammendola,
- Davide Badoni,
- Simona Bartocci,
- Stefania Beolè,
- Igor Bertello,
- William J. Burger,
- Donatella Campana,
- Antonio Cicone,
- Piero Cipollone,
- Silvia Coli,
- Livio Conti,
- Andrea Contin,
- Marco Cristoforetti,
- Fabrizio De Angelis,
- Cinzia De Donato,
- Cristian De Santis,
- Andrea Di Luca,
- Emiliano Fiorenza,
- Francesco Maria Follega,
- Giuseppe Gebbia,
- Roberto Iuppa,
- Alessandro Lega,
- Mauro Lolli,
- Bruno Martino,
- Matteo Martucci,
- Giuseppe Masciantonio,
- Matteo Mergè,
- Marco Mese,
- Alfredo Morbidini,
- Coralie Neubüser,
- Francesco Nozzoli,
- Fabrizio Nuccilli,
- Alberto Oliva,
- Giuseppe Osteria,
- Francesco Palma,
- Federico Palmonari,
- Beatrice Panico,
- Emanuele Papini,
- Alexandra Parmentier,
- Stefania Perciballi,
- Francesco Perfetto,
- Alessio Perinelli,
- Piergiorgio Picozza,
- Michele Pozzato,
- Gianmaria Rebustini,
- Dario Recchiuti,
- Ester Ricci,
- Marco Ricci,
- Sergio B. Ricciarini,
- Andrea Russi,
- Zuleika Sahnoun,
- Umberto Savino,
- Valentina Scotti,
- Xuhui Shen,
- Alessandro Sotgiu,
- Roberta Sparvoli,
- Silvia Tofani,
- Nello Vertolli,
- Veronica Vilona,
- Vincenzo Vitale,
- Ugo Zannoni,
- Simona Zoffoli,
- Paolo Zuccon
Affiliations
- Mirko Piersanti
- Department of Physical and Chemical Sciences, University of L’Aquila
- Pietro Ubertini
- National Institute of Astrophysics, IAPS
- Roberto Battiston
- Department of Physics, University of Trento
- Angela Bazzano
- National Institute of Astrophysics, IAPS
- Giulia D’Angelo
- National Institute of Astrophysics, IAPS
- James G. Rodi
- National Institute of Astrophysics, IAPS
- Piero Diego
- National Institute of Astrophysics, IAPS
- Zhima Zeren
- National Institute of Natural Hazards, Ministry of Emergency Management of China
- Roberto Ammendola
- INFN, University of Rome Tor Vergata
- Davide Badoni
- INFN, University of Rome Tor Vergata
- Simona Bartocci
- INFN, University of Rome Tor Vergata
- Stefania Beolè
- INFN - Sezione di Torino
- Igor Bertello
- National Institute of Astrophysics, IAPS
- William J. Burger
- TIFPA-INFN, Povo
- Donatella Campana
- INFN-Sezione di Napoli
- Antonio Cicone
- National Institute of Astrophysics, IAPS
- Piero Cipollone
- INFN, University of Rome Tor Vergata
- Silvia Coli
- INFN - Sezione di Torino
- Livio Conti
- INFN, University of Rome Tor Vergata
- Andrea Contin
- University of Bologna
- Marco Cristoforetti
- TIFPA-INFN, Povo
- Fabrizio De Angelis
- National Institute of Astrophysics, IAPS
- Cinzia De Donato
- INFN, University of Rome Tor Vergata
- Cristian De Santis
- INFN, University of Rome Tor Vergata
- Andrea Di Luca
- Department of Physics, University of Trento
- Emiliano Fiorenza
- National Institute of Astrophysics, IAPS
- Francesco Maria Follega
- Department of Physics, University of Trento
- Giuseppe Gebbia
- Department of Physics, University of Trento
- Roberto Iuppa
- Department of Physics, University of Trento
- Alessandro Lega
- Department of Physics, University of Trento
- Mauro Lolli
- INFN - Sezione di Bologna
- Bruno Martino
- National Institute of Astrophysics, IAPS
- Matteo Martucci
- INFN, University of Rome Tor Vergata
- Giuseppe Masciantonio
- INFN, University of Rome Tor Vergata
- Matteo Mergè
- INFN, University of Rome Tor Vergata
- Marco Mese
- INFN-Sezione di Napoli
- Alfredo Morbidini
- National Institute of Astrophysics, IAPS
- Coralie Neubüser
- TIFPA-INFN, Povo
- Francesco Nozzoli
- TIFPA-INFN, Povo
- Fabrizio Nuccilli
- National Institute of Astrophysics, IAPS
- Alberto Oliva
- University of Bologna
- Giuseppe Osteria
- INFN-Sezione di Napoli
- Francesco Palma
- INFN, University of Rome Tor Vergata
- Federico Palmonari
- University of Bologna
- Beatrice Panico
- INFN-Sezione di Napoli
- Emanuele Papini
- National Institute of Astrophysics, IAPS
- Alexandra Parmentier
- National Institute of Astrophysics, IAPS
- Stefania Perciballi
- INFN - Sezione di Torino
- Francesco Perfetto
- INFN-Sezione di Napoli
- Alessio Perinelli
- Department of Physics, University of Trento
- Piergiorgio Picozza
- INFN, University of Rome Tor Vergata
- Michele Pozzato
- INFN - Sezione di Bologna
- Gianmaria Rebustini
- INFN, University of Rome Tor Vergata
- Dario Recchiuti
- National Institute of Astrophysics, IAPS
- Ester Ricci
- Department of Physics, University of Trento
- Marco Ricci
- INFN-LNF, Frascati
- Sergio B. Ricciarini
- IFAC-CNR
- Andrea Russi
- National Institute of Astrophysics, IAPS
- Zuleika Sahnoun
- INFN - Sezione di Bologna
- Umberto Savino
- INFN - Sezione di Torino
- Valentina Scotti
- INFN-Sezione di Napoli
- Xuhui Shen
- National Space Science Center, Chinese Academy of Sciences
- Alessandro Sotgiu
- INFN, University of Rome Tor Vergata
- Roberta Sparvoli
- INFN, University of Rome Tor Vergata
- Silvia Tofani
- National Institute of Astrophysics, IAPS
- Nello Vertolli
- National Institute of Astrophysics, IAPS
- Veronica Vilona
- Department of Physics, University of Trento
- Vincenzo Vitale
- INFN, University of Rome Tor Vergata
- Ugo Zannoni
- National Institute of Astrophysics, IAPS
- Simona Zoffoli
- Agenzia Spaziale Italia
- Paolo Zuccon
- Department of Physics, University of Trento
- DOI
- https://doi.org/10.1038/s41467-023-42551-5
- Journal volume & issue
-
Vol. 14,
no. 1
pp. 1 – 10
Abstract
Abstract 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).