Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity
International audience In this paper are described a new neutron spectrometer which operate in the Concordia station (Antarctica, Dome C) since December 2015. This instrument complements a network including neutron spectrometers operating in the Pic-du-Midi and the Pico dos Dias. Thus, this work pre...
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ftonera:oai:HAL:hal-01402881v1 2023-06-11T04:05:51+02:00 Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity Hubert, Guillaume ONERA - The French Aerospace Lab Toulouse ONERA 2016-07-15 https://hal.science/hal-01402881 https://doi.org/10.1016/j.astropartphys.2016.07.002 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2016.07.002 hal-01402881 https://hal.science/hal-01402881 doi:10.1016/j.astropartphys.2016.07.002 ISSN: 0927-6505 Astroparticle Physics https://hal.science/hal-01402881 Astroparticle Physics, 2016, 83, p. 30-39. ⟨10.1016/j.astropartphys.2016.07.002⟩ ATMOSPHERIC RADIATION ENVIRONMENT NEUTRON SPECTROMETER HIGH ALTITUDE STATIONS ANTARCTICA CONCORDIA STATION PIC DU MIDI STATION ATMORAD [PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] info:eu-repo/semantics/article Journal articles 2016 ftonera https://doi.org/10.1016/j.astropartphys.2016.07.002 2023-04-18T23:06:32Z International audience In this paper are described a new neutron spectrometer which operate in the Concordia station (Antarctica, Dome C) since December 2015. This instrument complements a network including neutron spectrometers operating in the Pic-du-Midi and the Pico dos Dias. Thus, this work present an analysis of cosmic ray induced-neutron based on spectrometers operated simultaneously in the Pic-du-Midi and the Concordia stations during a quiet solar activity. The both high station platforms allow for investigating the long period dynamics to analyze the spectral variation and effects of local and seasonal changes, but also the short term dynamics during solar flare events. A first part is devoted to analyze the count rates, the spectrum and the neutron fluxes, implying cross-comparisons between data obtained in the both stations. In a second part, measurements analyses were reinforced by modeling based on simulations of atmospheric cascades according to primary spectra which only depend on the solar modulation potential. Article in Journal/Newspaper Antarc* Antarctica ONERA: HAL (French Aerospace Lab) Concordia Station ENVELOPE(123.333,123.333,-75.100,-75.100) Astroparticle Physics 83 30 39 |
institution |
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ONERA: HAL (French Aerospace Lab) |
op_collection_id |
ftonera |
language |
English |
topic |
ATMOSPHERIC RADIATION ENVIRONMENT NEUTRON SPECTROMETER HIGH ALTITUDE STATIONS ANTARCTICA CONCORDIA STATION PIC DU MIDI STATION ATMORAD [PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] |
spellingShingle |
ATMOSPHERIC RADIATION ENVIRONMENT NEUTRON SPECTROMETER HIGH ALTITUDE STATIONS ANTARCTICA CONCORDIA STATION PIC DU MIDI STATION ATMORAD [PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] Hubert, Guillaume Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity |
topic_facet |
ATMOSPHERIC RADIATION ENVIRONMENT NEUTRON SPECTROMETER HIGH ALTITUDE STATIONS ANTARCTICA CONCORDIA STATION PIC DU MIDI STATION ATMORAD [PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] |
description |
International audience In this paper are described a new neutron spectrometer which operate in the Concordia station (Antarctica, Dome C) since December 2015. This instrument complements a network including neutron spectrometers operating in the Pic-du-Midi and the Pico dos Dias. Thus, this work present an analysis of cosmic ray induced-neutron based on spectrometers operated simultaneously in the Pic-du-Midi and the Concordia stations during a quiet solar activity. The both high station platforms allow for investigating the long period dynamics to analyze the spectral variation and effects of local and seasonal changes, but also the short term dynamics during solar flare events. A first part is devoted to analyze the count rates, the spectrum and the neutron fluxes, implying cross-comparisons between data obtained in the both stations. In a second part, measurements analyses were reinforced by modeling based on simulations of atmospheric cascades according to primary spectra which only depend on the solar modulation potential. |
author2 |
ONERA - The French Aerospace Lab Toulouse ONERA |
format |
Article in Journal/Newspaper |
author |
Hubert, Guillaume |
author_facet |
Hubert, Guillaume |
author_sort |
Hubert, Guillaume |
title |
Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity |
title_short |
Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity |
title_full |
Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity |
title_fullStr |
Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity |
title_full_unstemmed |
Analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and Antarctica high-altitude stations during quiet solar activity |
title_sort |
analyses of cosmic ray induced-neutron based on spectrometers operated simultaneously at mid-latitude and antarctica high-altitude stations during quiet solar activity |
publisher |
HAL CCSD |
publishDate |
2016 |
url |
https://hal.science/hal-01402881 https://doi.org/10.1016/j.astropartphys.2016.07.002 |
long_lat |
ENVELOPE(123.333,123.333,-75.100,-75.100) |
geographic |
Concordia Station |
geographic_facet |
Concordia Station |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
ISSN: 0927-6505 Astroparticle Physics https://hal.science/hal-01402881 Astroparticle Physics, 2016, 83, p. 30-39. ⟨10.1016/j.astropartphys.2016.07.002⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2016.07.002 hal-01402881 https://hal.science/hal-01402881 doi:10.1016/j.astropartphys.2016.07.002 |
op_doi |
https://doi.org/10.1016/j.astropartphys.2016.07.002 |
container_title |
Astroparticle Physics |
container_volume |
83 |
container_start_page |
30 |
op_container_end_page |
39 |
_version_ |
1768377525182922752 |