Mesospheric ionization during substorm growth phase

Many studies have been conducted about the impact of energetic charged particles on the atmosphere during geomagnetically active times, while quiet time effects are poorly understood. We identified two energetic electron precipitation (EEP) events during the growth phase of moderate substorms and es...

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Main Authors: Murase Kiyoka, Kataoka Ryuho, Nishiyama Takanori, Nishimura Koji, Hashimoto Taishi, Tanaka Yoshimasa, Kadokura Akira, Tomikawa Yoshihiro, Tsutsumi Masaki, Ogawa Yasunobu, Uchida Herbert Akihito, Sato Kaoru, Kasahara Satoshi, Mitani Takefumi, Yokota Shoichiro, Hori Tomoaki, Keika Kunihiro, Takashima Takeshi, Kasahara Yoshiya, Matsuda Shoya, Shoji Masafumi, Matsuoka Ayako, Shinohara Iku, Miyoshi Yoshizumi, Sato Tatsuhiko, Ebihara Yusuke, Tanaka Takashi
Format: Article
Language:English
Published: EDP Sciences 2022-01-01
Series:Journal of Space Weather and Space Climate
Subjects:
Online Access:https://www.swsc-journal.org/articles/swsc/full_html/2022/01/swsc210073/swsc210073.html
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author Murase Kiyoka
Kataoka Ryuho
Nishiyama Takanori
Nishimura Koji
Hashimoto Taishi
Tanaka Yoshimasa
Kadokura Akira
Tomikawa Yoshihiro
Tsutsumi Masaki
Ogawa Yasunobu
Uchida Herbert Akihito
Sato Kaoru
Kasahara Satoshi
Mitani Takefumi
Yokota Shoichiro
Hori Tomoaki
Keika Kunihiro
Takashima Takeshi
Kasahara Yoshiya
Matsuda Shoya
Shoji Masafumi
Matsuoka Ayako
Shinohara Iku
Miyoshi Yoshizumi
Sato Tatsuhiko
Ebihara Yusuke
Tanaka Takashi
author_facet Murase Kiyoka
Kataoka Ryuho
Nishiyama Takanori
Nishimura Koji
Hashimoto Taishi
Tanaka Yoshimasa
Kadokura Akira
Tomikawa Yoshihiro
Tsutsumi Masaki
Ogawa Yasunobu
Uchida Herbert Akihito
Sato Kaoru
Kasahara Satoshi
Mitani Takefumi
Yokota Shoichiro
Hori Tomoaki
Keika Kunihiro
Takashima Takeshi
Kasahara Yoshiya
Matsuda Shoya
Shoji Masafumi
Matsuoka Ayako
Shinohara Iku
Miyoshi Yoshizumi
Sato Tatsuhiko
Ebihara Yusuke
Tanaka Takashi
author_sort Murase Kiyoka
collection DOAJ
description Many studies have been conducted about the impact of energetic charged particles on the atmosphere during geomagnetically active times, while quiet time effects are poorly understood. We identified two energetic electron precipitation (EEP) events during the growth phase of moderate substorms and estimated the mesospheric ionization rate for an EEP event for which the most comprehensive dataset from ground-based and space-born instruments was available. The mesospheric ionization signature reached below 70 km altitude and continued for ~15 min until the substorm onset, as observed by the PANSY radar and imaging riometer at Syowa Station in the Antarctic region. We also used energetic electron flux observed by the Arase and POES 15 satellites as the input for the air-shower simulation code PHITS to quantitatively estimate the mesospheric ionization rate. The calculated ionization level due to the precipitating electrons is consistent with the observed value of cosmic noise absorption. The possible spatial extent of EEP is estimated to be ~8 h MLT in longitude and ~1.5° in latitude from a global magnetohydrodynamic simulation REPPU and the precipitating electron observations by the POES satellite, respectively. Such a significant duration and spatial extent of EEP events suggest a non-negligible contribution of the growth phase EEP to the mesospheric ionization. Combining the cutting-edge observations and simulations, we shed new light on the space weather impact of the EEP events during geomagnetically quiet times, which is important to understand the possible link between the space environment and climate.
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spelling doaj.art-f6c88d8112d940c6bc31918e9749248a2022-12-22T00:27:13ZengEDP SciencesJournal of Space Weather and Space Climate2115-72512022-01-01121810.1051/swsc/2022012swsc210073Mesospheric ionization during substorm growth phaseMurase Kiyoka0https://orcid.org/0000-0001-8871-9199Kataoka Ryuho1https://orcid.org/0000-0001-9400-1765Nishiyama Takanori2https://orcid.org/0000-0002-3648-6589Nishimura Koji3https://orcid.org/0000-0001-8824-9844Hashimoto Taishi4https://orcid.org/0000-0002-7082-9530Tanaka Yoshimasa5Kadokura Akira6https://orcid.org/0000-0002-6105-9562Tomikawa Yoshihiro7https://orcid.org/0000-0002-5652-3017Tsutsumi Masaki8https://orcid.org/0000-0003-0113-8311Ogawa Yasunobu9https://orcid.org/0000-0002-8118-4475Uchida Herbert Akihito10https://orcid.org/0000-0002-4228-9178Sato Kaoru11Kasahara Satoshi12https://orcid.org/0000-0002-3479-772XMitani Takefumi13https://orcid.org/0000-0003-0492-3104Yokota Shoichiro14https://orcid.org/0000-0001-8851-9146Hori Tomoaki15https://orcid.org/0000-0001-8451-6941Keika Kunihiro16https://orcid.org/0000-0003-0265-4318Takashima Takeshi17https://orcid.org/0000-0002-7818-7800Kasahara Yoshiya18https://orcid.org/0000-0002-9304-8235Matsuda Shoya19https://orcid.org/0000-0003-4778-8897Shoji Masafumi20https://orcid.org/0000-0001-6573-525XMatsuoka Ayako21https://orcid.org/0000-0001-5777-9711Shinohara Iku22https://orcid.org/0000-0003-2700-0353Miyoshi Yoshizumi23https://orcid.org/0000-0001-7998-1240Sato Tatsuhiko24https://orcid.org/0000-0001-9902-7083Ebihara Yusuke25https://orcid.org/0000-0002-2293-1557Tanaka Takashi26Department of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIResearch Institute for Sustainable Humanosphere, Kyoto UniversityDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIDepartment of Polar Science, The Graduate University for Advanced Studies, SOKENDAIJapan Aerospace Exploration Agency, Institute of Space and Astronautical ScienceDepartment of Earth and Planetary Science, The University of TokyoDepartment of Earth and Planetary Science, The University of TokyoJapan Aerospace Exploration Agency, Institute of Space and Astronautical ScienceGraduate School of Science, Osaka UniversityInstitute for Space–Earth Environmental Research, Nagoya UniversityDepartment of Earth and Planetary Science, The University of TokyoJapan Aerospace Exploration Agency, Institute of Space and Astronautical ScienceGraduate School of Natural Science and Technology, Kanazawa UniversityGraduate School of Natural Science and Technology, Kanazawa UniversityInstitute for Space–Earth Environmental Research, Nagoya UniversityData Analysis Center for Geomagnetism and Space Magnetism, Kyoto UniversityJapan Aerospace Exploration Agency, Institute of Space and Astronautical ScienceInstitute for Space–Earth Environmental Research, Nagoya UniversityJapan Atomic Energy AgencyResearch Institute for Sustainable Humanosphere, Kyoto UniversityInternational Center for Space Weather Science and Education, Kyushu UniversityMany studies have been conducted about the impact of energetic charged particles on the atmosphere during geomagnetically active times, while quiet time effects are poorly understood. We identified two energetic electron precipitation (EEP) events during the growth phase of moderate substorms and estimated the mesospheric ionization rate for an EEP event for which the most comprehensive dataset from ground-based and space-born instruments was available. The mesospheric ionization signature reached below 70 km altitude and continued for ~15 min until the substorm onset, as observed by the PANSY radar and imaging riometer at Syowa Station in the Antarctic region. We also used energetic electron flux observed by the Arase and POES 15 satellites as the input for the air-shower simulation code PHITS to quantitatively estimate the mesospheric ionization rate. The calculated ionization level due to the precipitating electrons is consistent with the observed value of cosmic noise absorption. The possible spatial extent of EEP is estimated to be ~8 h MLT in longitude and ~1.5° in latitude from a global magnetohydrodynamic simulation REPPU and the precipitating electron observations by the POES satellite, respectively. Such a significant duration and spatial extent of EEP events suggest a non-negligible contribution of the growth phase EEP to the mesospheric ionization. Combining the cutting-edge observations and simulations, we shed new light on the space weather impact of the EEP events during geomagnetically quiet times, which is important to understand the possible link between the space environment and climate.https://www.swsc-journal.org/articles/swsc/full_html/2022/01/swsc210073/swsc210073.htmlmesospheric ionizationenergetic electron precipitationsubstormgrowth phase
spellingShingle Murase Kiyoka
Kataoka Ryuho
Nishiyama Takanori
Nishimura Koji
Hashimoto Taishi
Tanaka Yoshimasa
Kadokura Akira
Tomikawa Yoshihiro
Tsutsumi Masaki
Ogawa Yasunobu
Uchida Herbert Akihito
Sato Kaoru
Kasahara Satoshi
Mitani Takefumi
Yokota Shoichiro
Hori Tomoaki
Keika Kunihiro
Takashima Takeshi
Kasahara Yoshiya
Matsuda Shoya
Shoji Masafumi
Matsuoka Ayako
Shinohara Iku
Miyoshi Yoshizumi
Sato Tatsuhiko
Ebihara Yusuke
Tanaka Takashi
Mesospheric ionization during substorm growth phase
Journal of Space Weather and Space Climate
mesospheric ionization
energetic electron precipitation
substorm
growth phase
title Mesospheric ionization during substorm growth phase
title_full Mesospheric ionization during substorm growth phase
title_fullStr Mesospheric ionization during substorm growth phase
title_full_unstemmed Mesospheric ionization during substorm growth phase
title_short Mesospheric ionization during substorm growth phase
title_sort mesospheric ionization during substorm growth phase
topic mesospheric ionization
energetic electron precipitation
substorm
growth phase
url https://www.swsc-journal.org/articles/swsc/full_html/2022/01/swsc210073/swsc210073.html
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