SHIMOJO Masumi (下条 圭美)

Jets in the Solar Atmosphere

I have been trying to understand the release of magnetic energy in the solar atmosphere since I was an undergraduate student. Although it is well known that dynamic phenomena in the solar atmosphere are driven mainly by “magnetic reconnection,” it cannot explain everything. To fully explain these phenomena, we need to understand how magnetic energy is converted into thermal energy, plasma kinetic energy, and non-thermal-particle kinetic energy. To achieve my scientific goal, I am investigating jet phenomena in the solar atmosphere based on the observing data with a broad wavelength range, from radio to X-rays.

• X-ray jets in the north polar region
  observed with with the X-ray Telescope aboard Hinode satellite
• Recent refereed papers (as a coresponding author)
  • Shimojo et al. 2020, Astrophysical Journal Letters, 888, L28
    "Estimating the temperature and density of a spicule from 100 GHz data obtained with ALMA"
  • Shimojo et al. 2017, Astrophysical Journal Letters, 841, L5
    "The First ALMA Observation of a Solar Plasmoid Ejection from an X-Ray Bright Point"
  • Shimojo & Tsuneta 2009, Astrophysical Journal Letters, 706, p. L145
    "The Relation Between Magnetic Fields and Coronal Activities in the Polar Coronal Hole"
• Review paper (as a co-author)
  • Raouafi, et al. 2016, Space Science Reviews , 201, p. 1
    Solar Coronal Jets: Observations, Theory, and Modeling
• Scientific article written in Japanese (解説記事)
  • ひのでX線望遠鏡が見た太陽X線ジェット
    The Astronomical Herald, Jun. 2008

Observational Studies of Solar Cycle

The number of sunspots changes periodically, and its period is about 11 years. The fact is well known since the 18th century, but we cannot answer the question "Why sunspots change periodically?" yet. To solve the problem and understand the periodical variation of the solar atmosphere, I'm studying solar-cycle issues observationally, especially using solar radio data.

• Butterfly diagram created from the sites of the prominence eruptions observd with Nobeyama Radioheliograph (17 GHz)
• Recent refereed papers (as a corresponding author)
  • Shimojo et al. 2024, Astrophysical Journal, 965, 170
    "Comparison of solar multifrequency microwave data with other solar indices for understanding solar and stellar microwave data"
  • Shimojo et al. 2017, Astrophysical Journal, 848, 62
    "Variation of Solar Microwave Spectrum in the Last Half Century"
  • Shimojo 2013, Publications of the Astronomical Society of Japan, 65, S16
    "Unusual Migration of Prominence Activities in the Southern Hemisphere during Cycles 23-24"
• Scientific article written in Japanese (解説記事)
  • プロミネンス活動でみる太陽周期
    The Astronomical Herald, Aug. 2014
• Press Release
  • Solar Minimum Surprisingly Constant
    -More than Half a Century of Observation yields New Discovery-
    (17 Nov. 2017) WebPage: 日本語 / English
  • "Hinode" discovered strong magnetic field patches in the Sun's polar region.
    (9 Mar. 2010) WebPage: 日本語 / English

Solar Observations with ALMA

The Atacama Large Millimeter/submillimeter Array (ALMA) is the largest radio interferometer in the world for observing the celestial objects, mainly star formation region, high-z galaxy, molecular cloud. ALMA has a capacity of observing the Sun too, but the development of solar observations had not been done until 2010. We developed the solar observing method with Band3 (100 GHz) and Band6 (239 GHz) and started to offer solar observations to scientists in 2016. The development is continued for adding new functions of observing the Sun.

• Sunspot Observed with ALMA
  From Left: ALMA 239 GHz, SDO/AIA WL , SDO/AIA WL(Full Sun)
  
• Reference Papers
  • Shimojo et al. 2017, Solar Physics, 292, 87
    "Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): High-Resolution Interferometric Imaging"
    
  • White et al. 2017, Solar Physics, 292, 88
  "Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Fast-Scan Single-Dish Mapping"(as a co-author)
  • Shimojo et al. 2024, Solar Physics, 299,20
    "Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Polarization Observations at 3 mm"
    
• Review Paper (as a co-author)
  • Bastian, et al. 2022, Frontiers in Astronomy and Space Sciences, 9:977368
    Solar Observing with the Atacama Large Millimeter-Submillimeter Array
  • Nindos, et al. 2022, Frontiers in Astronomy and Space Sciences, 9:981205
    The dynamic chromosphere at millimeter wavelengths
  • Wedemeyer, et al. 2016, Space Science Reviews , 200, p. 1
    Solar Science with the Atacama Large Millimeter/Submillimeter Array — A New View of Our Sun
• Special Issue (as a guest editor)
  • "The Sun Seen with the Atacama Large mm and sub-mm Array (ALMA) - First Results", Frontiers in in Astronomy and Space Sciences
• Scientific article written in Japanese (解説記事)
  • アルマ望遠鏡による太陽観測
    The Astronomical Herald, May 2018
• Press Release
  • 2019 Solar Eclipse Image from ALMA. (3 Jul. 2019)
    WebPage: 日本語 / English
  • ALMA starts Observing the Sun. (18 Jan. 2017)
    WebPage: 日本語 / English
• Workshops for solar observations with ALMA
  • ALMA Solar Workshop Series (Written in Japanese)
  • 1st Interbational Workshop on Solar Imaging with ALMA
  • 2ns Interbational Workshop on Solar Imaging with ALMA
• Links
  • ALMA Observatory
  • ALMA Science Portal (EA)

Nobeyama Radio Polarimeters (NoRP)

Nobeyama Radio Polarimeters (NoRP) are observing the Sun with multiple frequencies in the microwave range. It is capable to obtain the total coming flux and the circular-polarization degree. The system of 17 GHz is routinely working since 1978, that of 35 GHz since 1983, and that of 80 GHz since 1984. The systems of 1, 2, 3.75, and 9.4 GHz were working at Toyokawa observatory of the Research Institute of Atmospherics, Nagoya University since the 1950s. They were moved to Nobeyama in Apr 1994 and has been working since then. I have been contributing to the operation of NoRP as a manager since 2019.

• Solar Cycle in Microwave (1951 - 2023)
  Blue: 1 GHz, Red: 2GHz, Orange: 3.75 GHz, Green 9.4 GHz,
  
• Reference Paper
  • Shimojo and Iwai 2023, Geoscience Data Journal, 10, 114–129
    "Over seven decades of solar microwave data obtained with Toyokawa and Nobeyama Radio Polarimeters"
• Link: Nobeyama Radio Polarimeters (NoRP)

"Hinode" Satellite (SOLAR-B)

The solar observing satellite “Hinode” was launched from Uchinoura Space Center on September 23, 2006 (JST). “Hinode” has three telescopes to observe the Sun. The cylindrical main body of the satellite is the Solar Optical Telescope (SOT) which observes in visible light. The cylinder attached beneath the main body is the X-Ray Telescope (XRT). The Extreme-ultraviolet Imaging Spectrometer (EIS) is mounted to the upper surface of the main body. These innovative telescopes can capture the movement of the complex solar magnetic fields and the three-dimensional motions of the plasma in real time.
I joined the Hinode project since 1999 and contributed the development of the X-Ray Telescope (XRT), Attitude Control System, Mission Operation and Data Analysis (MODA) and the establishing of Hinode Science Center at NAOJ. After launching "Hinode", I have been contributing to Public Outreach (2006 - 2013) and XRT Scientific Operation (2006 - present).

• X-Ray Sun observed with Hinode/XRT
  
　
• Reference Papers (as a co-author)
  • Kosugi et al. 2007, Solar Physics, 243, 3
    "The Hinode (Solar-B) Mission: An Overview"
  • Golub et al. 2007, Solar Physics, 243, 63
    "The X-Ray Telescope (XRT) for the Hinode Mission"
  • Matsuzaki et al. 2007, Solar Physics, 243, 87
    "Data Archive of the Hinode Mission"
  • Kano et al. 2008, Solar Physics, 249, 263
    "The Hinode X-Ray Telescope (XRT): Camera Design, Performance and Operations"
  • Narukage et al. 2011, Solar Physics, 269, 169
    "Coronal-Temperature-Diagnostic Capability of the Hinode/X-Ray Telescope Based on Self-Consistent Calibration"
  • Narukage et al. 2014, Solar Physics, 289, 1029
    "Coronal-Temperature-Diagnostic Capability of the Hinode/X-Ray Telescope Based on Self-consistent Calibration. II. Calibration with On-Orbit Data"
• Review Paper (as a co-author)
  • Hinode Review Team, et al. 2019, Publications of the Astronomical Society of Japan, 71, R1
    Achievements of Hinode in the First Eleven Years
• Articles written in Japanese (解説記事)
  • 「ひので」衛星の広報普及・教育活動
    The Astronomical Herald, Sep. 2016 (as a co-author)
  • ひのでサイエンスセンター -設立前から今後の課題まで-
    The Astronomical Herald, Oct. 2016
• Links
  • The solar observing satellite "Hinode"

"YOHKOH" Satellite (SOLAR-A)

"Yohkoh" is the 2nd solar observing satellite of Japan and was launched on 30 August 1991 (JST). The satellite's objectives were observations of solar flares during a maximum period of solar activity and revealed the physical mechanism of solar flares.
When I was an undergraduate student, I joined the Yohkoh project and started my career as a solar physics researcher. I investigated mainly solar X-ray jets discovered with Yohkoh satellite (Shibata et al. 1992 and Strong et al. 1992) and got a doctorate in March 1999.

• Final images observed with Soft X-ray Telescope aboard Yohkoh satellite (2001/12/15).
• My Doctoral Thesis
  • "Studies of Solar Coronal X-ray Jets"
    Supervisors: Prof. Kazunari Shibata & Prof. Tetsuya Watanabe
• Link: Yohkoh Homepage (written in Japanese)

Solar Data-Analysis Systems

For analyzing the solar data obtained with the solar telescopes on the ground and orbit, the computer system that is optimized for solar data-analysis is essential. I have contributed to the development and operation of the computer system for analyzing the data obtained with Hinode satellite, solar radio telescopes at Nobeyama and Yohkoh satellite, since when I was a graduate student.

• Current operated system: Solar Data Archive System (SDAS)
• Articles
  • First Ten Years of Hinode Solar On-Orbit Observatory
    2018, Astrophysics and Space Science Library, 449,
    [I took chrage of writing Chapter 22.]
  • ひのでサイエンスセンター -設立前から今後の課題まで-
    The Astronomical Herald, Oct. 2016
  • Shimojo & Tsuneta 2007, ASP Conference Series, Vol. 369, p.59
    "The Solar-B Science Center in Japan "
  • Shimojo 2007, ASP Conference Series, Vol. 369, p.31
    "Archiving, Distribution and Analysis of Solar-B Data"
  • Matsuzaki et al. 2007,Solar Physics, 292, 87
    "Data Archive of the Hinode Mission"
• Links
  • Astronomy Data Center
  • Solar Science Observatory
  • Data ARchive and Transmission System (DARTS), ISAS/JAXA

Publication

• Citation Metrics: Go to ADS (Only corresponding-author papers)
• 
• Web of Science ResearcherID: J-2605-2016
• Google Scholar: Masumi Shimojo
• Karadashian(K)-Index: 0.127 on 4 August 2023 (^^;;)
• Recent refereed papers (as a corresponding author)
  • Shimojo et al. 2024, Astrophysical Journal, 965, 170
    "Comparison of solar multifrequency microwave data with other solar indices for understanding solar and stellar microwave data"
  • Shimojo et al. 2024, Solar Physics, 299, 20
    "Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Polarization Observations at 3 mm"
    
  • Shimojo and Iwai 2023, Geoscience Data Journal, 10, 114–129
    "Over seven decades of solar microwave data obtained with Toyokawa and Nobeyama Radio Polarimeters"
• Review papers (as a co-author)
  • Bastian, et al. 2022, Frontiers in Astronomy and Space Sciences, 9:977368
    Solar Observing with the Atacama Large Millimeter-Submillimeter Array
  • Nindos, et al. 2022, Frontiers in Astronomy and Space Sciences, 9:981205
    The dynamic chromosphere at millimeter wavelengths
  • Hinode Review Team, et al. 2019, Publications of the Astronomical Society of Japan, 71, R1
    Achievements of Hinode in the First Eleven Years
  • Raouafi, et al. 2016, Space Science Reviews , 201, p. 1
    Solar Coronal Jets: Observations, Theory, and Modeling
  • Wedemeyer, et al. 2016, Space Science Reviews , 200, p. 1
    Solar Science with the Atacama Large Millimeter/Submillimeter Array — A New View of Our Sun
• Scientific papers in Japanese (解説記事)
  • アルマ望遠鏡による太陽観測
    The Astronomical Herald, May 2018
  • プロミネンス活動でみる太陽周期
    The Astronomical Herald, Aug. 2014
  • ひのでX線望遠鏡が見た太陽X線ジェット
    The Astronomical Herald, Jun. 2008

Teaching Experience

• Lectures for graduate/under-graduate students
  • Lecture “Astronomy I and II”
    at Faculty of Letters, Keio University (2019 - Present)
  • Face-2-Face Course "Basic of Observational Astronomy"
    at Gunma Study Center, The Open University of Japan
    (2019 - Present)
  • Lecture “Radio Astronomy I” at Astronomical Science Program,
    SOKENDAI (2nd Semester, 2023)
  • Spring School “Solar Physics”
    at SOKENDAI/NAOJ (Feb. 2018)
  • Intensive Course “Basic of Solar Physics”
    at Ibaraki University (Jul. 2013)
  • Intensive Course “Solar Eclipse”
    at Tokai University (Jun. 2008)
  • Intensive Course “Physics of Solar Atmosphere”
    at Ibaraki University (May 2008)
  • Intensive Course “Basic of Solar Physics”
    at Shiga University (Dec. 2002)
• Supervised Students
  • Ph.D. Students
    Nobuharu Sako, Sep. 2014, The graduate University of Advanced Studies
    "Statistical Study of X-ray Jets using Hinode/XRT"
  • Master Students
    Satoshi Kajita, Mar. 2015, Tokai University
    "A Study of Non-Thermal Particles before the Impulsive Phase of Solar Flares"
    Nobuharu Sako, Mar. 2011, Tokai University
    "ひので/XRTの観測データを用いた極域X線ジェットの統計的研究"
  • Under-graduate Students
    Satoshi Kajita, Mar. 2013, Tokai University
    "太陽フレアのプリフレア期における硬X線の研究"
    Daiki Ishikawa, Mar. 2009, Tokai University
    "ひので/SOTで見る太陽北極域の微細磁場構造とエフェメラルリージョン"
    Nobuharu Sako, Mar. 2009, Tokai University
    "太陽北極域で発生するX線ジェットの統計研究"

Public Outreach

• Lectures for general public
  • Jan. 2024
    Lecture at Tendai Elementary School, Ayase, Kanagawa
  • Dec. 2023
    Lecture at Tochigi Night Junior High School, Utunomiya Tochigi
  • Jan. 2023
    Lecture at MEISEI Junior and Senior High School , Fuchu, Tokyo
  • Nov. 2022
    Lecture at Moegino Elementary School , Yokohama, Kanagawa
  • Dec. 2021
    Lecture at Yamauchi Junior High School , Yokohama, Kanagawa
  • Nov. 2021
    Lecture at Tokai University Sagami Junior & Senior High School , Sagamihara, Kanagawa
  • May 2021
    Lecture at the founding ceremony of Utunomiya-Higashi Junior and Senior High School, Utunomiya, Tochigi
  • Jan. 2021
    Lecture at Asahi Culture Center/Yokohama, OnLine via Zoom
  • Nov. 2020
    Lecture at SOKENDAI/ISAS, OnLine via Zoom
  • Dec. 2019
    Lecture at Bosei Gakujyuku, Musashino, Tokyo
  • Nov. 2019
    Lecture at Ohshima Elementary School, Koriyama, Fukushima
  • Nov. 2019
    Lecture at MITA International School, Setagaya, Tokyo
  • Dec. 2018
    Short talk in the UNIVERSE Show at Science Museum, Chiyoda, Tokyo
  • Dec. 2018
    Lecture at Hachiouji Sanda Elementary School, Hachiouji, Tokyo
  • Nov. 2018
    Lecture at Sugatagawa Dai-ichi Elementary School, Utunomiya, Tochigi
  • Nov. 2017
    Lecture at Hadano Minami Junior High School, Hadano, Kanagawa
  • Oct. 2017
    Lecture at 2017 open-day of NAOJ, Mitaka, Tokyo
  • Sep. 2017
    Lecture at Yono-Hommachi Elementary School, Saitama, Saitama
  • Oct. 2016
    Lecture at Ohnohara Elementary School, Yamato, Kanagawa
  • Sep. 2016
    Lectures at Waseda open college (Nakano), Nakano, Tokyo
  • Jul. 2016
    Lectures at Kitakaruizawa-Sundai Astro. Summer School, Naganohara, Gunma
  • May 2016
    Short talk in the UNIVERSE Show at Science Museum, Chiyoda, Tokyo
  • Oct. 2015
    Lecture at Chofu-Otsuka Elementary School, Ota, Tokyo
  • Oct. 2015
    Lecture at Mejiro Elementary School, Toshima, Tokyo
  • Jul. 2014
    Lecture at Asahi Culture Center/Yokohama, Yokohama, Kanagawa
  • Mar. 2014
    Lecture at University of Shizuoka, Shizuoka, Shizuoka
  • Apr. 2012:
    Lecture at Asahi Culture Center/Yokohama, Yokohama, Kanagawa
  • Jan. 2010
    Lecture at Science Cafe OKAYAMA, Kurashiki, Okayama
  • Jul. 2009
    Lecture at Bosei Gakujyuku, Musasino, Tokyo
    
  • Jul. 2007
    Short talk in the UNIVERSE Show at Science Museum, Chiyoda,　Tokyo
  • Jun. 2006
    Lecture at Suginami Science Museum, Suginami, Tokyo
• Publications for general public
  • 文藝春秋5月号「同級生交歓」
    (文芸春秋社), 2020
  • 「We are 宇宙兄弟 宇宙を舞台に活躍する人たち」
    (講談社+α新書), 2012
  • 「皆既日食と宇宙のふしぎ―“謎”がいっぱいの宇宙を知ろう!」
    (SAKURA・MOOK 66), 2009
  • ひのでが拓く天文広報活動 SOKENDAI Journal, 2009, Vol. 16