Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations

International audience This work investigates solar events occurred in September 2017 characterized by a series of Forbush decreases and a ground level enhancement (GLE). Forbush decreases is a rapid decrease in the observed https://en.wikipedia.org/wiki/Galactic_cosmic_ray intensity following a cor...

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Published in:Journal of Geophysical Research: Space Physics
Main Authors: Hubert, Guillaume, Pazianotto, Maurizio T., Federico, Claudio Antonio, Ricaud, P.
Other Authors: ONERA / DPHY, Université de Toulouse Toulouse, ONERA-PRES Université de Toulouse, Instituto Tecnológico de Aeronáutica São José dos Campos (ITA), Instituto de Estudos Avançados (IEAV), Institut, Laboratoire d'aérologie (LAERO), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Météo-France Direction Interrégionale Sud-Est (DIRSE), Météo-France
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2019
Subjects:
Online Access:https://hal.science/hal-02346795
https://hal.science/hal-02346795/document
https://hal.science/hal-02346795/file/2018JA025834.pdf
https://doi.org/10.1029/2018JA025834
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author Hubert, Guillaume
Pazianotto, Maurizio T.
Federico, Claudio Antonio
Ricaud, P.
author2 ONERA / DPHY, Université de Toulouse Toulouse
ONERA-PRES Université de Toulouse
Instituto Tecnológico de Aeronáutica São José dos Campos (ITA)
Instituto de Estudos Avançados (IEAV)
Institut
Laboratoire d'aérologie (LAERO)
Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Météo-France Direction Interrégionale Sud-Est (DIRSE)
Météo-France
author_facet Hubert, Guillaume
Pazianotto, Maurizio T.
Federico, Claudio Antonio
Ricaud, P.
author_sort Hubert, Guillaume
collection Université de Nantes: HAL-UNIV-NANTES
container_issue 1
container_start_page 661
container_title Journal of Geophysical Research: Space Physics
container_volume 124
description International audience This work investigates solar events occurred in September 2017 characterized by a series of Forbush decreases and a ground level enhancement (GLE). Forbush decreases is a rapid decrease in the observed https://en.wikipedia.org/wiki/Galactic_cosmic_ray intensity following a coronal mass ejection while GLE is induced by a strong solar event for which the flux of high‐energy solar particles is sufficient to enhance the radiation level on the ground. These investigations were performed using data recorded by a neutron spectrometer network composed of a Bonner sphere system. Two instruments located at Pic‐du‐Midi Observatory (+2,885 m above sea level) and at Concordia station (Antarctica, +3,233 m) record simultaneously and continuously the neutron spectra, allowing to consider short‐term variations during solar events. The main objective is to analyze neutron spectral properties including their energy distributions and dynamics. This paper presents cosmic ray‐induced neutron spectra during active solar event leading to changes in the local cosmic ray spectrum (Forbush decreases and a GLE). Concerning the GLE, analyses show that neutrons in the evaporation domain are particularly amplified during the GLE, while other energetic domains increase uniformly.
format Article in Journal/Newspaper
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genre_facet Antarc*
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op_doi https://doi.org/10.1029/2018JA025834
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1029/2018JA025834
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Journal of Geophysical Research Space Physics, 2019, 124 (1), pp.661-673. ⟨10.1029/2018JA025834⟩
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spelling ftunivnantes:oai:HAL:hal-02346795v1 2025-01-16T19:04:39+00:00 Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations Hubert, Guillaume Pazianotto, Maurizio T. Federico, Claudio Antonio Ricaud, P. ONERA / DPHY, Université de Toulouse Toulouse ONERA-PRES Université de Toulouse Instituto Tecnológico de Aeronáutica São José dos Campos (ITA) Instituto de Estudos Avançados (IEAV) Institut Laboratoire d'aérologie (LAERO) Université Toulouse III - Paul Sabatier (UT3) Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS) Météo-France Direction Interrégionale Sud-Est (DIRSE) Météo-France 2019-01-22 https://hal.science/hal-02346795 https://hal.science/hal-02346795/document https://hal.science/hal-02346795/file/2018JA025834.pdf https://doi.org/10.1029/2018JA025834 en eng HAL CCSD American Geophysical Union/Wiley info:eu-repo/semantics/altIdentifier/doi/10.1029/2018JA025834 hal-02346795 https://hal.science/hal-02346795 https://hal.science/hal-02346795/document https://hal.science/hal-02346795/file/2018JA025834.pdf doi:10.1029/2018JA025834 info:eu-repo/semantics/OpenAccess ISSN: 2169-9380 EISSN: 2169-9402 Journal of Geophysical Research Space Physics https://hal.science/hal-02346795 Journal of Geophysical Research Space Physics, 2019, 124 (1), pp.661-673. ⟨10.1029/2018JA025834⟩ [SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere info:eu-repo/semantics/article Journal articles 2019 ftunivnantes https://doi.org/10.1029/2018JA025834 2023-02-22T04:18:52Z International audience This work investigates solar events occurred in September 2017 characterized by a series of Forbush decreases and a ground level enhancement (GLE). Forbush decreases is a rapid decrease in the observed https://en.wikipedia.org/wiki/Galactic_cosmic_ray intensity following a coronal mass ejection while GLE is induced by a strong solar event for which the flux of high‐energy solar particles is sufficient to enhance the radiation level on the ground. These investigations were performed using data recorded by a neutron spectrometer network composed of a Bonner sphere system. Two instruments located at Pic‐du‐Midi Observatory (+2,885 m above sea level) and at Concordia station (Antarctica, +3,233 m) record simultaneously and continuously the neutron spectra, allowing to consider short‐term variations during solar events. The main objective is to analyze neutron spectral properties including their energy distributions and dynamics. This paper presents cosmic ray‐induced neutron spectra during active solar event leading to changes in the local cosmic ray spectrum (Forbush decreases and a GLE). Concerning the GLE, analyses show that neutrons in the evaporation domain are particularly amplified during the GLE, while other energetic domains increase uniformly. Article in Journal/Newspaper Antarc* Antarctic Antarctica Université de Nantes: HAL-UNIV-NANTES Antarctic Concordia Station ENVELOPE(123.333,123.333,-75.100,-75.100) Journal of Geophysical Research: Space Physics 124 1 661 673
spellingShingle [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
Hubert, Guillaume
Pazianotto, Maurizio T.
Federico, Claudio Antonio
Ricaud, P.
Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations
title Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations
title_full Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations
title_fullStr Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations
title_full_unstemmed Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations
title_short Analysis of the Forbush Decreases and Ground‐Level Enhancement on September 2017 Using Neutron Spectrometers Operated in Antarctic and Midlatitude Stations
title_sort analysis of the forbush decreases and ground‐level enhancement on september 2017 using neutron spectrometers operated in antarctic and midlatitude stations
topic [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
topic_facet [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
url https://hal.science/hal-02346795
https://hal.science/hal-02346795/document
https://hal.science/hal-02346795/file/2018JA025834.pdf
https://doi.org/10.1029/2018JA025834