Profile (English)

Full CV (as of Nov 13, 2025) can be downloaded from here.

Personal Details

Email

Research Interests

Academic positions

   Laboratory for Atmospheric and Space Physics (LASP) , University of Colorado Boulder (CU Boulder)   

          Also affiliated with National Solar Observatory  (NSO, located in LASP)

      Laboratory for Atmospheric and Space Physics (LASP), University of Colorado Boulder (CU Boulder)

      Also affiliated with National Solar Observatory (NSO, located in LASP)

    [1] Laboratory for Atmospheric and Space Physics (LASP), University of Colorado Boulder (CU Boulder)

            Also affiliated with National Solar Observatory (NSO, located in LASP)

                                  [2] Department of Earth and Planetary Sciences, School of Science, Tokyo Institute of Technology (Tokyo Tech)

                                       (Long-term staying at LASP/CU, Early termination on 2023.03 because I moved completely to the US institution)

      Laboratory for Atmospheric and Space Physics (LASP), University of Colorado Boulder (CU Boulder)

      Also affiliated with National Solar Observatory (NSO, located in LASP)

                                              Department of Astronomy, Graduate School of Science, Kyoto University 

Education

                                              Department of Astronomy, Graduate School of Science, Kyoto University 

                                              Ph. D. thesis "Observational studies on solar-type superflare stars"  doi:10.14989/doctor.k21575)

                                             Department of Astronomy, Graduate School of Science, Kyoto University 

                                             Master Thesis: "High dispersion spectroscopy of solar-type superflare stars"

                                             Department of Astronomy, Faculty of Science, Kyoto University

Honors & Awards

Grants (PI ones are mainly listed)

                              “Solar-Like Periodic Modulations And Flare Emissions From The Nearest Neighbour Proxima Centauri”

                                              NNH24ZDA001N-LWS (PI, $986.1K, ID: 24-LWS24_2-0044), Also selected to be the Focused Science Team Lead

                                              “Comparison of stellar steady state and transient phenomena affecting planetary atmospheric escape and habitability”

                                            “High-Time Resolution Multi-Color Properties of Stellar Flares on G-M Dwarfs”

                   “Simultaneous SWIFT/UVOT NUV Photometry with the HST Treasury Program NUV Spectroscopy and TESS Photometry”

                  “Simultaneous X-ray Monitoring of M Dwarf Flares with the HST Treasury Program NUV Spectroscopy and TESS Photometry”

                                   “High-Time Resolution Multi-Color Properties of Stellar Flares”

Professional Service

   Membership

   Service

   International teams

   International Conference/Workshop Organizer