Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»

The barometric effect of cosmic ray neutron component was estimated on the example of the Antarctic station Mirny. We used hourly data from continuous monitoring of neutron component and data from a local weather station for 2007–2014. Wind speed at the station Mirny reaches 20–40 m/s in winter that...

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Main Authors: Kobelev P.G., Аbunin А.А., Аbunina M.А., Preobrazhensky M.S., Smirnov D.V., Lukovnikova А.А.
Format: Article
Language:English
Published: INFRA-M 2016-03-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/ru/nauka/article/12019/view
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author Kobelev P.G.
Аbunin А.А.
Аbunina M.А.
Preobrazhensky M.S.
Smirnov D.V.
Lukovnikova А.А.
author_facet Kobelev P.G.
Аbunin А.А.
Аbunina M.А.
Preobrazhensky M.S.
Smirnov D.V.
Lukovnikova А.А.
author_sort Kobelev P.G.
collection DOAJ
description The barometric effect of cosmic ray neutron component was estimated on the example of the Antarctic station Mirny. We used hourly data from continuous monitoring of neutron component and data from a local weather station for 2007–2014. Wind speed at the station Mirny reaches 20–40 m/s in winter that corresponds to the dynamic pressure 5–6 mbar and leads to a 5 % error in variations of neutron component because of dynamic effects in the atmosphere. The results can be applied to detectors located in high-latitude and high-mountain regions where the wind speed can be significant.
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spelling doaj.art-ef9c09cd7afe45cd8c4b471fa8486a6d2022-12-21T21:52:54ZengINFRA-MSolar-Terrestrial Physics2500-05352016-03-01219710210.12737/19882Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»Kobelev P.G.0Аbunin А.А.1Аbunina M.А.2Preobrazhensky M.S.3Smirnov D.V.4Lukovnikova А.А.5Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Troitsk, Moscow, RussiaPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Troitsk, Moscow, RussiaPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Troitsk, Moscow, RussiaPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Troitsk, Moscow, RussiaPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS, Troitsk, Moscow, RussiaInstitute of Solar-Terrestrial Physics SB RAS, Irkutsk, RussiaThe barometric effect of cosmic ray neutron component was estimated on the example of the Antarctic station Mirny. We used hourly data from continuous monitoring of neutron component and data from a local weather station for 2007–2014. Wind speed at the station Mirny reaches 20–40 m/s in winter that corresponds to the dynamic pressure 5–6 mbar and leads to a 5 % error in variations of neutron component because of dynamic effects in the atmosphere. The results can be applied to detectors located in high-latitude and high-mountain regions where the wind speed can be significant.https://naukaru.ru/ru/nauka/article/12019/viewgalactic cosmic ray variationsbarometric effectneutron monitors
spellingShingle Kobelev P.G.
Аbunin А.А.
Аbunina M.А.
Preobrazhensky M.S.
Smirnov D.V.
Lukovnikova А.А.
Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»
Solar-Terrestrial Physics
galactic cosmic ray variations
barometric effect
neutron monitors
title Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»
title_full Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»
title_fullStr Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»
title_full_unstemmed Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»
title_short Barometric effect of neutron component of cosmic rays at Antarctic station «Mirny»
title_sort barometric effect of neutron component of cosmic rays at antarctic station mirny
topic galactic cosmic ray variations
barometric effect
neutron monitors
url https://naukaru.ru/ru/nauka/article/12019/view
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