Updated on 2025/11/20

写真a

 
Kita Hajime
 
Organization
- - Lecturer
External link

Degree

  • 博士(理学) ( 2015.3   東北大学 )

Research Interests

  • Radio Interferometer

  • Radiation Belt

  • Radio Telescope

  • Infrared Telescope

  • Jupiter

Research Areas

  • Natural Science / Space and planetary sciences

Papers

  • Results from Hisaki and prospects for LAPYUTA observations of the Jupiter System

    Fuminori Tsuchiya, Go Murakami, Atsushi Yamazaki, Kazuo Yoshioka, Masato Kagitani, Tomoki Kimura, Chihiro Tao, Ryoichi Koga, Hajime Kita, Jun Kimura, Shuya Tan, Kei Masunaga, Shotaro Sakai, Mizuki Yoneda, Masaki Kuwabara, Shingo Kameda, Ichiro Yoshikawa

    2025.3

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    Publisher:Copernicus GmbH  

    Remote sensing with ultraviolet wavelength (UV) are one of powerful probes to uncover dynamic behaviors of the planetary environment. The Hisaki satellite was an earth orbiting extreme ultraviolet (EUV) spectroscope dedicated for observing solar system planets. Thanks to its long-term monitoring capability, Hisaki had carried out unprecedented continuous observation of Io plasma torus, Jovian aurora, and Mars and Venus upper atmospheres from 2013 to 2023. One of notable phenomena observed by Hisaki is significant enhancements of neutral gas from presumed activation of volcanic activity on Io. Hisaki revealed, for the first time, that not only the plasma source, but transport, heating, and loss processes of magnetospheric plasma were influenced by the variation in the neutral source input.After the end of the Hisaki mission, we have proposed the next UV space telescope, LAPYUTA (Life-environmentology, Astronomy, and PlanetarY Ultraviolet Telescope Assembly). One of goals of this mission is dynamics of our solar system planets and moons as the most quantifiable archetypes of extraterrestrial habitable environments in the universe. LAPYUTA will not only provide a UV monitoring platform like Hisaki but also have a high spatial resolution and high sensitivity to uncover stability of Io’s atmosphere, water plumes that gushes from the subsurface ocean of icy moons, and spatio-temporal aspects of Jupiter's giant UV aurora. Primary goal of the LAPYUTA mission other than the Jovian system includes atmospheric evolution of Venus and Mars, characterization of exoplanet atmosphere, galaxy formation, and time-domain astronomy.

    DOI: 10.5194/egusphere-egu25-14544

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  • Solar wind response of the dawn-dusk asymmetry in the Io plasma torus using the Haleakala T60 and HISAKI satellite observations

    Hiroyasu Kondo, Fuminori Tsuchiya, Masato Kagitani, Shinnosuke Satoh, Hiroaki Misawa, Yuki Nakamura, Go Murakami, Tomoki Kimura, Atsushi Yamazaki, Ichiro Yoshikawa, Hajime Kita, Chihiro Tao

    2024.5

  • A search for auroral radio emission from β Pictoris b

    Yuta Shiohira, Yuka Fujii, Hajime Kita, Tomoki Kimura, Yuka Terada, Keitaro Takahashi

    Monthly Notices of the Royal Astronomical Society   528 ( 2 )   2136 - 2144   2024.2

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1093/mnras/stad3990

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  • Simulation of Dawn‐To‐Dusk Electric Field in the Jovian Inner Magnetosphere via Region 2‐Like Field‐Aligned Current Reviewed

    Yuki Nakamura, Koichiro Terada, Chihiro Tao, Naoki Terada, Yasumasa Kasaba, François Leblanc, Hajime Kita, Aoi Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani, Fuminori Tsuchiya, Masato Kagitani, Takeshi Sakanoi, Go Murakami, Kazuo Yoshioka, Tomoki Kimura, Atsushi Yamazaki, Ichiro Yoshikawa

    Journal of Geophysical Research: Space Physics   128 ( 6 )   2023.6

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:American Geophysical Union (AGU)  

    DOI: 10.1029/2022ja031248

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  • Major results from the Hisaki mission and future perspectives

    Fuminori Tsuchiya, Yasumasa Kasaba, Ichiro Yoshikawa, Go Murakami, Atsushi Yamazaki, Kazuo Yoshioka, Tomoki Kimura, Chihiro Tao, Ryoichi Koga, Hajime Kita, Kei Masunaga, Masato Kagitani, Shotaro Sakai, Masaki Kuwabara

    2023.2

  • Effect of Meteoric Ions on Ionospheric Conductance at Jupiter

    Yuki Nakamura, Koichiro Terada, Chihiro Tao, Naoki Terada, Yasumasa Kasaba, François Leblanc, Hajime Kita, Aoi Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani, Fuminori Tsuchiya, Masato Kagitani, Takeshi Sakanoi, Go Murakami, Kazuo Yoshioka, Tomoki Kimura, Atsushi Yamazaki, Ichiro Yoshikawa

    Journal of Geophysical Research: Space Physics   127 ( 3 )   2022.3

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    Publishing type:Research paper (scientific journal)   Publisher:American Geophysical Union (AGU)  

    DOI: 10.1029/2022ja030312

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    Other Link: https://onlinelibrary.wiley.com/doi/full-xml/10.1029/2022JA030312

  • Jupiter's X-ray aurora during UV dawn storms and injections as observed by XMM-Newton, Hubble, and Hisaki

    A. D. Wibisono, G. Branduardi-Raymont, W. R. Dunn, T. Kimura, A. J. Coates, D. Grodent, Z. H. Yao, H. Kita, P. Rodriguez, G. R. Gladstone, B. Bonfond, R. P. Haythornthwaite

    Monthly Notices of the Royal Astronomical Society   507 ( 1 )   1216 - 1228   2021.10

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1093/mnras/stab2218

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  • Variation of Jupiter's Aurora Observed by Hisaki/EXCEED: 4. Quasi‐Periodic Variation

    Chihiro Tao, Tomoki Kimura, Elena A. Kronberg, Fuminori Tsuchiya, Go Murakami, Atsushi Yamazaki, Marissa F. Vogt, Bertrand Bonfond, Kazuo Yoshioka, Ichiro Yoshikawa, Yasumasa Kasaba, Hajime Kita, Shogo Okamoto

    Journal of Geophysical Research: Space Physics   126 ( 2 )   2021.2

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    Publishing type:Research paper (scientific journal)   Publisher:American Geophysical Union (AGU)  

    DOI: 10.1029/2020ja028575

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    Other Link: https://onlinelibrary.wiley.com/doi/full-xml/10.1029/2020JA028575

  • Long‐Term Monitoring of Energetic Protons at the Bottom of Earth’s Radiation Belt

    K. Yoshioka, Y. Miyoshi, S. Kurita, M. Teramoto, F. Tsuchiya, A. Yamazaki, G. Murakami, T. Kimura, H. Kita, I. Yoshikawa, Y. Kasaba

    Space Weather   19 ( 1 )   2021.1

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    Publishing type:Research paper (scientific journal)   Publisher:American Geophysical Union (AGU)  

    DOI: 10.1029/2020sw002611

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    Other Link: https://onlinelibrary.wiley.com/doi/full-xml/10.1029/2020SW002611

  • The Formation of Saturn’s and Jupiter’s Electron Radiation Belts by Magnetospheric Electric Fields

    Yi-Xin Hao, Yi-Xin Sun, Elias Roussos, Ying Liu, Peter Kollmann, Chong-Jing Yuan, Norbert Krupp, Chris Paranicas, Xu-Zhi Zhou, Go Murakami, Hajime Kita, Qiu-Gang Zong

    The Astrophysical Journal   905 ( 1 )   L10 - L10   2020.12

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    Publishing type:Research paper (scientific journal)   Publisher:American Astronomical Society  

    DOI: 10.3847/2041-8213/abca3f

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    Other Link: https://iopscience.iop.org/article/10.3847/2041-8213/abca3f

  • An attempt to detect transient changes in Io’s SO2 and NaCl atmosphere

    Lorenz Roth, Jeremie Boissier, Arielle Moullet, Álvaro Sánchez-Monge, Katherine de Kleer, Mizuki Yoneda, Reina Hikida, Hajime Kita, Fuminori Tsuchiya, Aljona Blöcker, G. Randall Gladstone, Denis Grodent, Nickolay Ivchenko, Emmanuel Lellouch, Kurt D. Retherford, Joachim Saur, Peter Schilke, Darrell Strobel, Sven Thorwirth

    Icarus   350   113925 - 113925   2020.11

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    Publishing type:Research paper (scientific journal)   Publisher:Elsevier BV  

    DOI: 10.1016/j.icarus.2020.113925

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  • Spatially Asymmetric Increase in Hot Electron Fraction in the Io Plasma Torus During Volcanically Active Period Revealed by Observations by Hisaki/EXCEED From November 2014 to May 2015 Reviewed

    R. Hikida, K. Yoshioka, F. Tsuchiya, M. Kagitani, T. Kimura, F. Bagenal, N. Schneider, G. Murakami, A. Yamazaki, H. Kita, E. Nerney, I. Yoshikawa

    Journal of Geophysical Research: Space Physics   2020.3

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1029/2019ja027100

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  • Jovian UV Aurora's Response to the Solar Wind: Hisaki EXCEED and Juno Observations Reviewed

    H. Kita, T. Kimura, C. Tao, F. Tsuchiya, G. Murakami, A. Yamazaki, K. Yoshioka, R.W. Ebert, R.J. Wilson, F. Allegrini, G. Clark, J. E. P. Connerney, G. R. Gladstone, I. Yoshikawa, M. Fujimoto

    Journal of Geophysical Research: Space Physics   2019.12

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    Authorship:Lead author   Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1029/2019ja026997

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  • Short-term Variation in the Dawn–Dusk Asymmetry of the Jovian Radiation Belt Obtained from GMRT and Hisaki EXCEED Observations Reviewed

    H. Kita, H. Misawa, A. Bhardwaj, F. Tsuchiya, G. Murakami, C. Tao, T. Kimura, K. Yoshioka, A. Yamazaki, Y. Kasaba, I. Yoshikawa, M. Fujimoto

    The Astrophysical Journal   2019.2

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/2041-8213/ab0427

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  • Two-element radio interferometer for the observation of Jupiter's synchrotron radiation Reviewed

    Fuminori Tsuchiya, Hiroaki Misawa, Hajime Kita, Akira Morioka, Tetsuro Kondo

    Proceedings of the International Symposium on Planetary Science 2011   47 - 58   2019

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    Language:English   Publishing type:Research paper (international conference proceedings)  

    DOI: 10.5047/pisps.047

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  • Development of ground pipeline system for high-level scientific data products of the Hisaki satellite mission and its application to planetary space weather Reviewed

    Tomoki Kimura, Atsushi Yamazaki, Kazuo Yoshioka, Go Murakami, Fuminori Tsuchiya, Hajime Kita, Chihiro Tao, Ichiro Yoshikawa, Atsushi Kumamoto, Chisato Yamauchi

    Journal of Space Weather and Space Climate   2019

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    Publishing type:Research paper (scientific journal)  

    <jats:p>The Hisaki satellite is the first-ever space telescope mission dedicated to planetary sciences. Atmospheres and magnetospheres of our solar system planets are continuously monitored by the extreme ultraviolet (EUV) spectrometer onboard Hisaki. This paper describes a data pipeline system developed for processing high-level scientific and ancillary data products from the Hisaki mission. The telemetry data downlinked from the satellite are stored in a ground telemetry database, processed in the pipeline to imaging spectral data with a 1-min temporal resolution and ancillary data products, and then archived in a public database. The imaging spectra can be further reduced to higher-level data products for practical scientific use. For example, light curves of the power emitted from Jupiter’s aurora and plasma torus with a temporal resolution of 10-min can be reduced from the imaging spectral data; the reduced light curves reveal the transport processes of energy and mass in Jupiter’s magnetosphere and associated interplanetary solar wind conditions. Continuous monitoring with Hisaki will contribute considerably to our understanding of space weather relating to planets in our solar system.</jats:p>

    DOI: 10.1051/swsc/2019005

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  • Impact of Io's volcanic activity to environment and dynamics in the Jovian magnetosphere : from HISAKI results

    Tsuchiya, F, K. Yoshioka, T. Kimura, G. Murakami, A. Yamazaki, M. Kagitani, C. Tao, H. Kita, R. Koga, F. Suzuki, R. Hikida, Y. Kasaba, H. Misawa, T. Sakanoi, I. Yoshikawa

    Proceedings of Symposium on Planetary Science 2019   2019

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    Language:English   Publishing type:Research paper (international conference proceedings)  

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  • Pulsation Characteristics of Jovian Infrared Northern Aurora Observed by the Subaru IRCS with Adaptive Optics Reviewed

    H. Watanabe, H. Kita, C. Tao, M. Kagitani, T. Sakanoi, Y. Kasaba

    Geophysical Research Letters   2018.11

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1029/2018gl079411

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  • Investigating Solar Wind‐Driven Electric Field Influence on Long‐Term Dynamics of Jovian Synchrotron Radiation Reviewed

    S. Han, G. Murakami, H. Kita, F. Tsuchiya, C. Tao, H. Misawa, A. Yamazaki, M. Nakamura

    Journal of Geophysical Research: Space Physics   2018.11

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1029/2018ja025849

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  • Study of the Solar Wind Influence on the Jovian Inner Magnetosphere Using an Ionospheric Potential Solver

    K Terada, C Tao, N Terada, Y Kasaba, H Kita, A Nakamizo, A Yoshikawa, S Ohtani, F Tsuchiya, M Kagitani, T Sakanoi, G Murakami, K Yoshioka, T Kimura, A Yamazaki, I Yoshikawa

    Proceeding of Lunar and Planetary Science Conference   49   2018.10

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    Language:English   Publishing type:Research paper (scientific journal)  

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  • Horizontal and vertical structures of Jovian infrared aurora: Observation using Subaru IRCS with adaptive optics Reviewed

    Hajime Kita, Shota Fujisawa, Chihiro Tao, Masato Kagitani, Takeshi Sakanoi, Yasumasa Kasaba

    Icarus   2018.10

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1016/j.icarus.2018.05.002

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  • Enhancement of the Jovian Magnetospheric Plasma Circulation Caused by the Change in Plasma Supply From the Satellite Io Reviewed

    F. Tsuchiya, K. Yoshioka, T. Kimura, R. Koga, G. Murakami, A. Yamazaki, M. Kagitani, C. Tao, F. Suzuki, R. Hikida, I. Yoshikawa, Y. Kasaba, H. Kita, H. Misawa, T. Sakanoi

    Journal of Geophysical Research: Space Physics   2018.8

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1029/2018ja025316

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  • Response of Jupiter's Aurora to Plasma Mass Loading Rate Monitored by the Hisaki Satellite During Volcanic Eruptions at Io Reviewed

    T. Kimura, Y. Hiraki, C. Tao, F. Tsuchiya, P. A. Delamere, K. Yoshioka, G. Murakami, A. Yamazaki, H. Kita, S. V. Badman, K. Fukazawa, I. Yoshikawa, M. Fujimoto

    Journal of Geophysical Research: Space Physics   2018.3

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/2017ja025029

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  • Variation of Jupiter's Aurora Observed by Hisaki/EXCEED: 3. Volcanic Control of Jupiter's Aurora Reviewed

    Chihiro Tao, Tomoki Kimura, Fuminori Tsuchiya, Go Muirakami, Kazuo Yoshioka, Atsushi Yamazaki, Sarah V. Badman, Hiroaki Misawa, Hajime Kita, Yasumasa Kasaba, Ichiro Yoshikawa, Masaki Fujimoto

    Geophysical Research Letters   2018.1

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/2017gl075814

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  • Feasibility of the exploration of the subsurface structures of Jupiter's icy moons by interference of Jovian hectometric and decametric radiation Reviewed

    Kumamoto, A, Y. Kasaba, F. Tsuchiya, H. Misawa, H. Kita, W. Puccio, J.-E. Wahlund, J. Bergman, B. Cecconi, Y. Goto, J. Kimura, T. Kobayashi

    Planetary Radio Emissions VIII, edited by G. Fischer, G. Mann, M. Panchenko, and P. Zarka, Austrian Academy of Sciences Press, Vienna   127 - 136   2017.8

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    Language:English   Publishing type:Research paper (international conference proceedings)  

    DOI: 10.1553/PRE8s127

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  • Volcanic activity on Io and its influence on the dynamics of the Jovian magnetosphere observed by EXCEED/Hisaki in 2015 Reviewed

    Ichiro Yoshikawa, Fumiharu Suzuki, Reina Hikida, Kazuo Yoshioka, Go Murakami, Fuminori Tsuchiya, Chihiro Tao, Atsushi Yamazaki, Tomoki Kimura, Hajime Kita, Hiromasa Nozawa, Masaki Fujimoto

    EARTH PLANETS AND SPACE   69   2017.8

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1186/s40623-017-0700-9

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  • A flux comparison of northern and southern Saturn kilometric radio bursts during southern summer Reviewed

    Kasaba, Y, T. Kimura, D. Maruno, A. Morioka, B. Cecconi, L. Lamy, C. M. Jackman, C. Tao, H. Kita, H. Misawa, T. Tsuchiya, A. Kumamoto

    Planetary Radio Emissions VIII, edited by G. Fischer, G. Mann, M. Panchenko, and P. Zarka, Austrian Academy of Sciences Press, Vienna   205 - 215   2017.8

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    Language:English   Publishing type:Research paper (international conference proceedings)  

    DOI: 10.1553/PRE8s205

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  • Transient brightening of Jupiter's aurora observed by the Hisaki satellite and Hubble Space Telescope during approach phase of the Juno spacecraft Reviewed

    T. Kimura, J. D. Nichols, R. L. Gray, C. Tao, G. Murakami, A. Yamazaki, S. V. Badman, F. Tsuchiya, K. Yoshioka, H. Kita, D. Grodent, G. Clark, I. Yoshikawa, M. Fujimoto

    GEOPHYSICAL RESEARCH LETTERS   44 ( 10 )   4523 - 4531   2017.5

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:AMER GEOPHYSICAL UNION  

    In early 2014, continuous monitoring with the Hisaki satellite discovered transient auroral emission at Jupiter during a period when the solar wind was relatively quiet for a few days. Simultaneous imaging made by the Hubble Space Telescope (HST) suggested that the transient aurora is associated with a global magnetospheric disturbance that spans from the inner to outer magnetosphere. However, the temporal and spatial evolutions of the magnetospheric disturbance were not resolved because of the lack of continuous monitoring of the transient aurora simultaneously with the imaging. Here we report the coordinated observation of the aurora and plasma torus made by Hisaki and HST during the approach phase of the Juno spacecraft in mid-2016. On day 142, Hisaki detected a transient aurora with a maximum total H-2 emission power of similar to 8.5 TW. The simultaneous HST imaging was indicative of a large "dawn storm," which is associated with tail reconnection, at the onset of the transient aurora. The outer emission, which is associated with hot plasma injection in the inner magnetosphere, followed the dawn storm within less than two Jupiter rotations. The monitoring of the torus with Hisaki indicated that the hot plasma population increased in the torus during the transient aurora. These results imply that the magnetospheric disturbance is initiated via the tail reconnection and rapidly expands toward the inner magnetosphere, followed by the hot plasma injection reaching the plasma torus. This corresponds to the radially inward transport of the plasma and/or energy from the outer to the inner magnetosphere.

    DOI: 10.1002/2017GL072912

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  • ひさき衛星を用いた木星紫外オーロラの太陽風応答に関する統計解析

    2017

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  • Three-year of observations of Jupiter's aurora and Io plasma torus variabilities by earth orbiting extreme-ultraviolet spectroscope HISAKI Reviewed

    F. Tsuchiya, K. Yoshioka, T. Kimura, G. Murakami, C. Tao, H. Kita, I. Yoshikawa, A. Yamazaki, Y. Kasaba

    FRONTIERS IN THEORETICAL AND APPLIED PHYSICS/UAE 2017 (FTAPS 2017)   869 ( 1 )   UNSP 012069   2017

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    Language:English   Publishing type:Research paper (international conference proceedings)  

    DOI: 10.1088/1742-6596/869/1/012069

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    Other Link: http://orcid.org/0000-0002-8160-3553

  • WIDE-BAND SPECTRA of GIANT RADIO PULSES from the CRAB PULSAR Reviewed

    Ryo Mikami, Katsuaki Asano, Shuta J. Tanaka, Shota Kisaka, Mamoru Sekido, Kazuhiro Takefuji, Hiroshi Takeuchi, Hiroaki Misawa, Fuminori Tsuchiya, Hajime Kita, Yoshinori Yonekura, Toshio Terasawa

    Astrophysical Journal   832 ( 2 )   2016.12

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/0004-637X/832/2/212

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  • Response of Jupiter's inner magnetosphere to the solar wind derived from extreme ultraviolet monitoring of the Io plasma torus Reviewed

    Go Murakami, Kazuo Yoshioka, Atsushi Yamazaki, Fuminori Tsuchiya, Tomoki Kimura, Chihiro Tao, Hajime Kita, Masato Kagitani, Takeshi Sakanoi, Kazunori Uemizu, Yasumasa Kasaba, Ichiro Yoshikawa, Masaki Fujimoto

    GEOPHYSICAL RESEARCH LETTERS   43 ( 24 )   12308 - 12316   2016.12

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/2016GL071675

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  • Wide-Band Spectra of Giant Radio Pulses from the Crab Pulsar Reviewed

    Ryo Mikami, Katsuaki Asano, Shuta J. Tanaka, Shota Kisaka, Mamoru Sekido, Kazuhiro Takefuji, Hiroshi Takeuchi, Hiroaki Misawa, Fuminori Tsuchiya, Hajime Kita, Yoshinori Yonekura, Toshio Terasawa

    2016.8

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    We present the results of the simultaneous observation of the giant radio
    pulses (GRPs) from the Crab pulsar at 0.3, 1.6, 2.2, 6.7, and 8.4 GHz with four
    telescopes in Japan. We obtain 3194 and 272 GRPs occurring at the main pulse
    and the interpulse phases, respectively. A few GRPs detected at both 0.3 and
    8.4 GHz are the most wide-band samples ever reported. In the frequency range
    from 0.3 to 2.2 GHz, we find that about 70\% or more of the GRP spectra are
    consistent with single power laws and the spectral indices of them are
    distributed from $-4$ to $-1$. We also find that a significant number of GRPs
    have such a hard spectral index (approximately $-1$) that the fluence at 0.3
    GHz is below the detection limit ("dim-hard" GRPs). Stacking light curves of
    such dim-hard GRPs at 0.3 GHz, we detect consistent enhancement compared to the
    off-GRP light curve. Our samples show apparent correlations between the
    fluences and the spectral hardness, which indicates that more energetic GRPs
    tend to show softer spectra. Our comprehensive studies on the GRP spectra are
    useful materials to verify the GRP model of fast radio bursts in future
    observations.

    DOI: 10.3847/0004-637X/832/2/212

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  • Very Long Baseline Interferometry Experiment on Giant Radio Pulses of Crab Pulsar toward Fast Radio Burst Detection Reviewed

    K. Takefuji, T. Terasawa, T. Kondo, R. Mikami, H. Takeuchi, H. Misawa, F. Tsuchiya, H. Kita, M. Sekido

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC   128 ( 966 )   2016.8

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1088/1538-3873/128/966/084502

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  • Characteristics of solar wind control on Jovian UV auroral activity deciphered by long-term Hisaki EXCEED observations: Evidence of preconditioning of the magnetosphere? Reviewed

    Hajime Kita, Tomoki Kimura, Chihiro Tao, Fuminori Tsuchiya, Hiroaki Misawa, Takeshi Sakanoi, Yasumasa Kasaba, Go Murakami, Kazuo Yoshioka, Atsushi Yamazaki, Ichiro Yoshikawa, Masaki Fujimoto

    Geophysical Research Letters   2016.7

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/2016gl069481

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  • Relation between the short-term variation of the Jovian radiation belt and thermosphere derived from radio and infrared observations Reviewed

    Kita Hajime, Misawa Hiroaki, Bhardwaj Anil, Tsuchiya Fuminori, Sakanoi Takeshi, Kasaba Yasumasa, Tao Chihiro, Miyoshi Yoshizumi, Morioka Akira

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   120 ( 8 )   6614 - 6623   2015.8

  • Relation between the short‐term variation of the Jovian radiation belt and thermosphere derived from radio and infrared observations Reviewed

    Hajime Kita, Hiroaki Misawa, Anil Bhardwaj, Fuminori Tsuchiya, Takeshi Sakanoi, Yasumasa Kasaba, Chihiro Tao, Yoshizumi Miyoshi, Akira Morioka

    Journal of Geophysical Research: Space Physics   2015.8

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/2015ja021374

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  • Vertical emissivity profiles of Jupiter's northern H-3(+) and H-2 infrared auroras observed by Subaru/IRCS Reviewed

    T. Uno, Y. Kasaba, C. Tao, T. Sakanoi, M. Kagitani, S. Fujisawa, H. Kita, S. V. Badman

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   119 ( 12 )   2014.12

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/2014JA020454

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  • Response of the Jovian thermosphere to variations in solar EUV flux Reviewed

    Chihiro Tao, Yoshizumi Miyoshi, Nick Achilleos, Hajime Kita

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   119 ( 5 )   3664 - 3682   2014.5

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:AMER GEOPHYSICAL UNION  

    Examining the response to solar extreme ultraviolet (EUV) radiation is an established diagnostic method used to understand the physics of planetary environments. In this study, we focus on the response of the Jovian thermosphere to variations in the solar EUV flux and discuss the consequences for the coupled thermosphere-ionosphere-magnetosphere system. We use a model that simulates both the thermospheric dynamics and the magnetospheric plasma velocity distribution under conditions of angular momentum transport between these regions. The simulations show that when the EUV flux increases by similar to 100% and 200%, the thermospheric neutral wind velocity at similar to 45 degrees latitude increases by 16% and 22%, respectively. The short-term variation over a few Earth days causes an increased velocity at middle latitudes which are magnetically conjugate to the Jovian radiation belt. Increased heating due to solar EUV contributes to this velocity change. The other contribution arises similar to 30 planetary rotations after the initial solar EUV flux increase. This second (delayed) effect is due to propagation of momentum from high latitudes (the auroral region), where Joule heating is dominant, and is related to the behavior of the ionospheric conductance and magnetosphere-ionosphere coupling currents. The modeled velocity enhancement is smaller than that required to explain the observed enhancement of the synchrotron emission by radial diffusion of the trapped energetic electrons. In this context, we discuss the sensitivity of the underlying thermosphere-ionosphere response to short-wavelength solar radiation and the ensuing three-dimensional wind fields.

    DOI: 10.1002/2013JA019411

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  • Response of the Jovian thermosphere to variations in solar EUV flux Reviewed

    Chihiro Tao, Yoshizumi Miyoshi, Nick Achilleos, Hajime Kita

    Journal of Geophysical Research: Space Physics   119 ( 5 )   3664 - 3682   2014

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Blackwell Publishing Ltd  

    DOI: 10.1002/2013JA019411

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  • Observations of Infrared and Synchrotron Emission from Jupiter during Sprint-A/EXCEED Campaign

    Kita, H, H. Misawa, F. Tsuchiya, S. Fujisawa, T. Sakanoi, Y. Kasaba

    2014惑星圏研究会集録   2014

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    Language:Japanese   Publishing type:Research paper (other academic)  

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  • Effect of solar UV/EUV heating on the intensity and spatial distribution of Jupiter's synchrotron radiation Reviewed

    H. Kita, H. Misawa, F. Tsuchiya, C. Tao, A. Morioka

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   118 ( 10 )   6106 - 6115   2013.10

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    Language:English   Publishing type:Research paper (scientific journal)  

    DOI: 10.1002/jgra.50568

    Web of Science

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  • Effect of solar UV/EUV heating on the intensity and spatial distribution of Jupiter's synchrotron radiation Reviewed

    H. Kita, H. Misawa, F. Tsuchiya, C. Tao, A. Morioka

    Journal of Geophysical Research: Space Physics   118 ( 10 )   6105 - 6115   2013

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    Language:English   Publishing type:Research paper (scientific journal)   Publisher:Blackwell Publishing Ltd  

    DOI: 10.1002/jgra.50568

    Scopus

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  • Two-element radio interferometer for the observation of Jupiter's synchrotron radiation Reviewed

    Tsuchiya, F, H. Misawa, H. Kita, A. Morioka, T. Kondo

    Proc. International Symposium on Planetary Science 2011   2013

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    Language:English   Publishing type:Research paper (international conference proceedings)  

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Research Projects

  • 宇宙・地上望遠鏡・探査機・及びモデルを融合させた木星磁気圏の粒子加速に関する研究

    Grant number:19H01948  2019.4 - 2022.3

    日本学術振興会  科学研究費助成事業  基盤研究(B)

    吉岡 和夫, 山崎 敦, 土屋 史紀, 木村 智樹, 北 元, 垰 千尋

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    Grant amount:\16900000 ( Direct Cost: \13000000 、 Indirect Cost:\3900000 )

    本年度の繰り越し分の経費を用いて,イオ火山の活発化に伴うイオプラズマトーラスの高温電子輸送のパラメタ特定,とくに朝夕非対称性について議論を深めることができた.
    具体的には,ひさき衛星のデータの中から,5つのイオ火山イベントに関連するデータを抽出し,それらに対してスペクトルフィッティング手法を通してプラズマの密度および温度を導出する手法を確立した.これまでは,頻度の低い高分解モードでのスペクトルにしか適応できなかったこのパラメタ導出を,広視野(低分解能)モードのデータにも適用可能になる手法を確立したことにより,プラズマパラメタの導出を時間軸に拡張することに成功した.
    NASAのJuno探査機の研究チームのその場観測データと,米国コロラド大学の研究チームが開発しているモデルを組み合わせることで,ひさき衛星のデータから導出したパラメタとの整合性を確認できた.ただし,NASA/Juno探査機の高エネルギー電子やイオン観測装置などによる,木星内部磁気圏のその場観測データの解析に関しては,当初想定していたほどの進捗は見られなかった.これは主にCOVID-19による海外渡航の制限が主な原因であるが,今後は遠隔体制でも効率よくデータ解析できるシステムを構築する.また,小研究会の開催などを通して引き続き米国の研究チームと密に連絡を取り合うことで,校正データの共有などを高頻度で進める.なお,今年度の研究成果として国際学術論文誌2編と博士論文1件,修士論文4件が発表された.

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