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’n‹…“dŽ¥‹CE’n‹…˜f¯Œ—Šw‰ï@Šw¶”­•\ÜiƒI[ƒƒ‰ƒƒ_ƒ‹j
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SGEPSS Student Presentation Award (Aurora Medal)

‘æ152‰ñu‰‰‰ï (2022”N) | ‘æ150‰ñu‰‰‰ï (2021”N) | ‘æ148‰ñu‰‰‰ï (2020”N) | ‘æ146‰ñu‰‰‰ï (2019”N) | ‘æ144‰ñu‰‰‰ï (2018”N) | ‘æ142‰ñu‰‰‰ï (2017”N)
‘æ140‰ñu‰‰‰ï (2016”N) | ‘æ138‰ñu‰‰‰ï (2015”N) | ‘æ136‰ñu‰‰‰ï (2014”N) | ‘æ134‰ñu‰‰‰ï (2013”N)
‘æ132‰ñu‰‰‰ï (2012”N) | ‘æ130‰ñu‰‰‰ï (2011”N) | ‘æ128‰ñu‰‰‰ï (2010”N) | ‘æ126‰ñu‰‰‰ï (2009”N)
‘æ124‰ñu‰‰‰ï (2008”N) | ‘æ122‰ñu‰‰‰ï (2007”N) | ‘æ120‰ñu‰‰‰ï (2006”N) | ‘æ118‰ñu‰‰‰ï (2005”N)
‘æ116‰ñu‰‰‰ï (2004”N) |

H‚Ìu‰‰‰ï‚É‚¨‚¯‚éŠw¶”­•\‚ðR¸‚µA«—ˆ«A“Æ‘n«‚Ì‚ ‚錤‹†‚ðŒ°²‚µ‚Ü‚·B

ŽóÜŽÒ‚É‚ÍÜóAƒI[ƒƒ‰ƒƒ_ƒ‹A•›Ü‚ðt‚ÌSGEPSS‘‰ï‚Å‘¡’悵‚Ü‚·B

‘ÎÛ‚ÍAŠw¶‰ïˆõi”ŽŽm‰Û’öˆÈ‰ºAŒ¤‹†¶‚ðŠÜ‚ÞAPD‚ÍŠÜ‚Ü‚È‚¢j‚ª ‘æˆê’˜ŽÒ‚©‚”­•\ŽÒ‚Å‚ ‚é‘S‚Ä‚Ì”­•\‚Å‚·B

3‚‚̕ª–ì‚É•ª‚¯‚ÄR¸‚µA15-20–¼‚É1–¼’ö“x‚̔䗦‚ÅŽóÜŽÒ‚ð‘Io‚µ‚Ü‚·B ƒI[ƒ‰ƒ‹‚ƃ|ƒXƒ^[‚Í“¯ˆêŠî€‚Å•]‰¿‚µ‚Ü‚·B

ŽóÜ”­•\ˆÈŠO‚ÌŠw¶”­•\‚ðŠÜ‚ÞŠe•ª–ì‚ɂ‚¢‚Ä‚ÌÚ‚µ‚¢u•]‚ªR¸ˆõ‚É‚æ‚Á‚Ä‚È‚³‚ê‚Ü‚·B

ŽóÜŒoŒ±ŽÒ‚Ì”­•\‚àR¸‘ÎÛ‚Å‚·‚Ì‚ÅA•¡”‰ñ‚ÌŽóÜ‚à‰Â”\‚Å‚·B

Šw¶”­•\Ü‹K–ñ     


    ‘æ152‰ñu‰‰‰ï (2022”N11ŒŽ3“ú-11ŒŽ7“úFƒnƒCƒuƒŠƒbƒhŠJÃ)

    ŽóÜŽÒ | R¸ˆõ | •ª–ìu•] | Ž––±‹Ç

    ŽóÜŽÒ

      ’†‰Æ “¿^ (_ŒË‘åŠwF‘æ1•ª–ì)
        uƒ‰ƒEŠC–~‚É‚¨‚¯‚é’ªŽ¬‹NˆöŽ¥ê‚Ì3D ‡ŒvŽZv(R003-04)

      ˆÉ“¡ ‚ä‚è (“d‹C’ÊM‘åŠwF‘æ2•ª–ì)
        u‚ ‚点‰q¯A’nã‘S“VƒJƒƒ‰AEISCATƒŒ[ƒ_[‚É‚æ‚鎥‹C‹¤–𓯎žŠÏ‘ª‚ð—p‚¢‚½–¬“®ƒI[ƒƒ‰“dŽq‚̃Gƒlƒ‹ƒM[“Á«‚ÉŠÖ‚·‚錤‹†v(R005-19)

      ˜ú ˆÛ³ (‹ž“s‘åŠwF‘æ2•ª–ì)
        uStudy of nighttime midlatitude E-F coupling in geomagnetic conjugate regions using multi-source datav(R005-24)

      —é–Ø —Y‘å (“Œ‹ž‘åŠwF‘æ2•ª–ì)
        uœa¯‚̃Rƒ}’†‚̃‰ƒCƒ}ƒ“ƒ¿ü‚Ì•úŽË‹P“x•ª•z‚ɑ΂·‚錴ŽqŠÔÕ“Ë‚¨‚æ‚Ñ‘½dŽU—‚ÌŠñ—^v(R009-06)

      ‹g“c “Þ‰› (“Œ–k‘åŠwF‘æ2•ª–ì)
        uCO distributions and climatology in the Martian mesosphere and lower thermosphere retrieved from TGO NOMAD solar occultationviR009-19j

      ¬’J —ƒ (‹ž“s‘åŠwF‘æ3•ª–ì)
        uSimulation study of the harmonic structure of lower hybrid wave driven by energetic ions: comparison with observationviS001-26j

      “잊 ‘s‘¿ (“d‹C’ÊM‘åŠwF‘æ3•ª–ì)
        uAI ‚ƃWƒ“ƒoƒ‹‚ð—p‚¢‚½ƒAƒNƒeƒBƒu‚ȃI[ƒƒ‰ŠÏ‘ªƒVƒXƒeƒ€‚ÌŠJ”­‚Ɖ^—pviR006-15j

    R¸ˆõ

      ŽsŒ´ Š°i–¼ŒÃ‰®‘åŠwF‘æ1•ª–ì)
      ”nê ¹ŽŠi“Œ‹ž‘åŠwF‘æ1•ª–ì)
      쑺 ‹IŽqiŠCã•ÛˆÀ’¡F‘æ1•ª–ì)
      ’†“c —T”Viç—t‘åŠwF‘æ2•ª–ìR005‘ã•\j
      “cŒû ^i—§‹³‘åŠwF‘æ2•ª–ìR009‘ã•\j
      Huixin Liui‹ãB‘åŠwF‘æ2•ª–ìj
      •iì —T”Viî•ñ’ÊMŒ¤‹†‹@\F‘æ2•ª–ìj
      쌴 ‘ô–çiMB‘åŠwF‘æ2•ª–ì)
      ’Óc ‘ì—Yi“d‹C’ÊM‘åŠwF‘æ2•ª–ì)
      ¼‰ª ÊŽqi‹ž“s‘åŠwF‘æ2•ª–ì)
      –ìŒû Žsi“Þ—Ç—Žq‘åŠwF‘æ2•ª–ì)
      –Ø‘º ’qŽ÷i“Œ‹ž—‰È‘åŠwF‘æ2•ª–ì)
      ‹g‰ª ˜a•vi“Œ‹ž‘åŠwF‘æ2•ª–ì)
      _ŽR “OiŽY‹Æ‹Zp‘‡Œ¤‹†ŠF‘æ2•ª–ì)
      ŽO‘î —m•½i_ŒË‘åŠwF‘æ3•ª–ìS001iR007AR008j‘ã•\)
      ŠC˜VŒ´ —S•ãi‹ž“s‘åŠwF‘æ3•ª–ìR006-1‘ã•\j
      –x ’qºi–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìR006-2 ‘ã•\)
      ¼’J –]i–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìR010‘ã•\)
      ó‘º ˜aŽji‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ3•ª–ì)
      “V–ì FLi“Œ‹ž‘åŠwF‘æ3•ª–ì)
      ¡é si‹ž“s‘åŠwF‘æ3•ª–ì)
      Šâˆä ˆê³i–¼ŒÃ‰®‘åŠwF‘æ3•ª–ì)
      ”~“c —²si–¼ŒÃ‰®‘åŠwF‘æ3•ª–ì)
      Š}Œ´ Œdi“Œ‹ž‘åŠwF‘æ3•ª–ìj
      •—ŠÔ —mˆêiASIAAF‘æ3•ª–ì)
      –k‘º Œ’‘¾˜Yi‹ãBH‹Æ‘åŠwF‘æ3•ª–ì)
      ‰–ì ˜a•vi–¼ŒÃ‰®‘åŠwF‘æ3•ª–ì)
      ŽÂŒ´ ˆçi‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ3•ª–ì)
      ‚‹´ ’¼Žqiî•ñ’ÊMŒ¤‹†‹@\F‘æ3•ª–ì)
      ‰i‰ª Œ«ˆêiŠj—Z‡‰ÈŠwŒ¤‹†ŠF‘æ3•ª–ì)
      ’†–ì T–çi“Œv”—Œ¤‹†ŠF‘æ3•ª–ì)
      ¼–ì ^–Øi“Œ‹ž‘åŠwF‘æ3•ª–ì)
      •½Œ´ ¹•¶i–¼ŒÃ‰®‘åŠwF‘æ3•ª–ì)
      ×ì Œh—Si“d‹C’ÊM‘åŠwF‘æ3•ª–ì)
      ŽR–{ ˜aOi“Œ‹ž‘åŠwF‘æ3•ª–ì)
      ‹gì Œ°³i‹ãB‘åŠwF‘æ3•ª–ì)

    •ª–ìu•]

      ‘æ‚P•ª–ì
      u’n‹…E˜f¯“à•”“dŽ¥‹CŠwi“d‹C“`“±“xA’nŠkŠˆ“®“dŽ¥‹CŠwjvAu’nŽ¥‹CEŒÃ’nŽ¥‹CEŠâÎŽ¥‹Cv
      ‘æ‚Q•ª–ì
      u‘å‹CŒ—E“d—£Œ—vAu˜f¯Œ—E¬“V‘Ìv
      ‘æ‚R•ª–ì
      u“Á•ÊƒZƒbƒVƒ‡ƒ“FSGEPSSE“V•¶Šw‰ïE•¨—Šw‰ï‡“¯ƒZƒbƒVƒ‡ƒ“:Žº“àŽÀŒ±E˜f¯E“V‘̃vƒ‰ƒYƒ}‚Ì••Õ«‚Æ‘½—l«vAuŽ¥‹CŒ—vAu‘¾—zŒ—vAu‰F’ˆƒvƒ‰ƒYƒ}—˜_EƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“vAu‰F’ˆ“V‹CE‰F’ˆ‹CŒó`ŠÏ‘ªAƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“A‚»‚Ì—Z‡v

    Ž––±‹Ç

      “ì‘ñli_ŒË‘åŠwF‘æ1•ª–ìj
      ‰Á“¡çŒbi‹ãB‘åŠwF‘æ1•ª–ìj
      ²ì‰p•vi‹ž“sŽY‹Æ‘åŠwF‘æ2•ª–ìj
      •äÏ—T‘¾iî•ñ’ÊMŒ¤‹†‹@\F‘æ2•ª–ìj
      ‚‹´“§i“dŽqq–@Œ¤‹†ŠF‘æ2•ª–ìj
      ¼“c¸–çi‹à‘ò‘åŠwF‘æ3•ª–ìj
      Ž›–{–œ—¢Žqi‹ãBH‹Æ‘åŠwF‘æ3•ª–ìj
      ŒI“c—åi‹ž“s‘åŠwF‘æ3•ª–ìj
      Œ´“c—TŒÈi‹ž“s‘åŠwF‘æ3•ª–ìj
      ŽOD—Rƒi–¼ŒÃ‰®‘åŠwFŽ––±‹Ç’·j
      ŽR’J—S‰îiŽY‹Æ‹Zp‘‡Œ¤‹†ŠF•›Ž––±‹Ç’·)
      ˆ¢•”CŽii‹ãB‘åŠwF•›Ž––±‹Ç’·)
      ‘å–î_‘ãiç—t‘åŠwF•›Ž––±‹Ç’·)
      ‰Pˆä—mˆêi‹à‘ò‘åŠwF•›Ž––±‹Ç’·)

      ‘æ150‰ñu‰‰‰ï (2021”N11ŒŽ1“ú-11ŒŽ4“úFƒIƒ“ƒ‰ƒCƒ“ŠJÃ)

      ŽóÜŽÒ | R¸ˆõ | •ª–ìu•] | Ž––±‹Ç

      ŽóÜŽÒ

        ‰ð—Ç ‘ñŠC (“Œ–k‘åŠwF‘æ1•ª–ì)
          uEnergy transfer among the equatorially symmetric components of magnetic and flow fields during dipole reversals in geodynamo modelv(R004-03)

        쑺 ”ü‹G (“Œ–k‘åŠwF‘æ2•ª–ì)
          uSimultaneous pulsating aurora and microburst observations with ground-based fast auroral imagers and CubeSat FIREBIRD-IIv(R005-04)

        ì‡ q‹P (–¼ŒÃ‰®‘åŠwF‘æ2•ª–ì)
          u’nã‚Æ‚ ‚点‰q¯‚É‚æ‚é–éŠÔ’†‹K–Í“`”À«“d—£Œ—ï—‚Ì•¡”—ᓯŽžŠÏ‘ªv(R005-11)

        ’†‘º —E‹M (“Œ–k‘åŠwF‘æ2•ª–ì)
          uNumerical prediction of changes in atmospheric compositions during SEP events at Marsv(R009-31)

        âV“¡ K× (“Œ–k‘åŠwF‘æ3•ª–ì)
          uŽ¥‹CÔ“¹Žü•Ó‚Å‚Ìkinetic Alfven wave‚É‚æ‚é“dŽq‰Á‘¬‰ß’ö‚ÉŠÖ‚·‚éƒeƒXƒg—±ŽqŒvŽZviR006-16j

        ›¶ ^ (“Œ‹ž‘åŠwF‘æ3•ª–ì)
          u«—ˆ‚̘f¯’T¸‚ÉŒü‚¯‚½ASIC‹Zp‚É‚æ‚é10-100 keV“dŽqŠÏ‘ªŠí‚̬Œ^‰»viR006-47j

        ’†‘º Kô (–¼ŒÃ‰®‘åŠwF‘æ3•ª–ì)
          u‚Š´“x‘S“VƒJƒƒ‰‚ÆVan Allen Probes‰q¯‚É‚æ‚éƒTƒuƒI[ƒƒ‰‘ьǗ§ƒvƒƒgƒ“ƒI[ƒƒ‰‚Ì•¡”—ᓯŽžŠÏ‘ªviR006-66j

        ŽRì ’qŽk (“Œ‹ž‘åŠwF‘æ3•ª–ì)
          uTwo types of storm-time Pc5 ULF waves excited in the Magnetosphere-Ionosphere coupled modelviR006-14j

      R¸ˆõ

        ‘å–ì ³•vi‹ãB‘åŠwF‘æ1•ª–ìj
        ‹g‘º —ߌdi‹ž“s‘åŠwF‘æ1•ª–ìj
        Ö“¡ ‹i“dŽqq–@Œ¤‹†ŠF‘æ2•ª–ìR005‘ã•\j
        ²“¡ Œõ‹Pi–kŠC“¹‘åŠwF‘æ2•ª–ìR009‘ã•\j
        ¡‘º „i“Œ‹ž‘åŠwF‘æ2•ª–ìj
        ¼–ì ^–Øi‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ2•ª–ìj
        –Ø‘º ’qŽ÷i“Œ‹ž—‰È‘åŠwF‘æ2•ª–ìj
        –ìàV Œå“¿i–¼ŒÃ‰®‘åŠwF‘æ2•ª–ìj
        ŽOD •×Mi‹ãB‘åŠwF‘æ2•ª–ìj
        w‰p Žiî•ñ’ÊMŒ¤‹†‹@\F‘æ2•ª–ìj
        ŠC˜VŒ´ —S•ã(‹ž“s‘åŠwF‘æ3•ª–ìR006-2‘ã•\)
        ‰Æ“c ͳ(–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìR006-3‘ã•\)
        ¬s ‘×—T (•xŽR‘åŠwF‘æ3•ª–ìR007/R008‘ã•\)
        âŒû ‰ÌD (î•ñ’ÊMŒ¤‹†‹@\F‘æ3•ª–ìR006-1/R010‘ã•\)
        –å‘q ºi‘—§‹É’nŒ¤‹†ŠF‘æ3•ª–ìj
        –k‘º ¬Žõi“Œ‹ž‘åŠwF‘æ3•ª–ìj
        ꎓ¡ TŽiiî•ñ’ÊMŒ¤‹†‹@\F‘æ3•ª–ìj
        ¬˜H ^Žji–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìj
        ”\¨ ³mi–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìj
        ]•› —Sˆê˜Yi“Œ‹ž“s—§‘åŠwF‘æ3•ª–ìj
        ”ö‰Ô —R‹Ii‘åã“d’Ê‘åŠwF‘æ3•ª–ìj
        Š}Œ´ Œdi“Œ‹ž‘åŠwF‘æ3•ª–ìj
        •—ŠÔ —mˆêi‘ä˜p’†‰›Œ¤‹†‰@F‘æ3•ª–ìj
        ‰Í–ì ‰pºi‹ãB‘åŠwF‘æ3•ª–ìj
        “cŒû ‘i‹ž“s‘åŠwF‘æ3•ª–ìj
        ’r“c º‘åiŽ­Ž™“‡‚êF‘æ3•ª–ìj
        ¡é si‹ž“s‘åŠwF‘æ3•ª–ìj
        –k‘º Œ’‘¾˜Yi‹ãBH‹Æ‘åŠwF‘æ3•ª–ìj
        ’†–ì T–çi“Œv”—Œ¤‹†ŠF‘æ3•ª–ìj
        ¼’J –]i–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìj
        “V–ì FLi“Œ‹ž‘åŠwF‘æ3•ª–ìj
        ”~“c —²si–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìj
        –kŒ´ —Oi–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìj
        “¿ŠÛ @—˜i–¼ŒÃ‰®‘åŠwF‘æ3•ª–ìj
        ’†‘º ‰ë•vi‘åã•{—§‘åŠwF‘æ3•ª–ìj
        ŽRè “Öi‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ3•ª–ìj

      •ª–ìu•]

        ‘æ1•ª–ì
        u’n‹…E˜f¯“à•”“dŽ¥‹CŠwi“d‹C“`“±“xA’nŠkŠˆ“®“dŽ¥‹CŠwjvAu’nŽ¥‹CEŒÃ’nŽ¥‹CEŠâÎŽ¥‹Cv
        ‘æ2•ª–ì
        u‘å‹CŒ—E“d—£Œ—vAu˜f¯Œ—E¬“V‘Ìv
        ‘æ3•ª–ì
        uŽ¥‹CŒ—vAu‘¾—zŒ—vAu‰F’ˆƒvƒ‰ƒYƒ}—˜_EƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“vAu‰F’ˆ“V‹CE‰F’ˆ‹CŒó`ŠÏ‘ªAƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“A‚»‚Ì—Z‡v

      Ž––±‹Ç

        ŽOD —Rƒi–¼ŒÃ‰®‘åŠwFŽ––±‹Ç’·j
        ŽR’J —S‰îiŽY‹Æ‹Zp‘‡Œ¤‹†ŠFŽ––±‹Çj
        ˆ¢•” CŽi (‹ãB‘åŠwFŽ––±‹Çj
        ‘å–î _‘ã (ç—t‘åŠwFŽ––±‹Ç)
        ‰Pˆä —mˆê (ŠC—mŒ¤‹†ŠJ”­‹@\FŽ––±‹Ç)
        “ì ‘ñli_ŒË‘åŠwF‘æ1•ª–ìj
        ²“¡ ‰ë•Fi“Œ‹ž‘åŠwF‘æ1•ª–ìj
        ²ì ‰p•vi‹ž“sŽY‹Æ‘åŠwF‘æ2•ª–ìj
        ²“¡ —²—Yi–kŠC“¹î•ñ‘åŠwF‘æ2•ª–ìj
        ‚‹´ “§i“dŽqq–@Œ¤‹†ŠF‘æ2•ª–ìj
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        Ž›–{ –œ—¢Žqi‹ãBH‹Æ‘åŠwF‘æ3•ª–ìj
        ¼“c ¸–çi‹à‘ò‘åŠwF‘æ3•ª–ìj
        Œ´“c —TŒÈi‹ž“s‘åŠwF‘æ3•ª–ìj

      ‘æ148‰ñu‰‰‰ï (2020”N11ŒŽ1“ú-11ŒŽ4“úFƒIƒ“ƒ‰ƒCƒ“ŠJÃ)

      ŽóÜŽÒ | R¸ˆõ | •ª–ìu•] | Ž––±‹Ç

      ŽóÜŽÒ

        ”nê Í (•xŽmŽR‰ÈŠwŒ¤‹†ŠEŒF–{‘åŠwF‘æ1•ª–ì)
          u•xŽmŽR‚É‚¨‚¯‚é‹IŒ³‘O1000”N‚©‚ç¼—ï1100”N‚É‚©‚¯‚Ä‚Ì’nŽ¥‹C‰i”N•Ï‰»‹Èüv(R004-01)

        ¼“ˆ —È (“d‹C’ÊM‘åŠwF‘æ2•ª–ì)
          uPropagation characteristics of Sporadic-E and MSTIDs: Statistics using HF Doppler and GPS-TEC datav(R005-43)

        ‹{–{ –¾•à (“Œ–k‘åŠwF‘æ2•ª–ì)
          uIntense zonal wind in the Martian mesosphere during the 2018 planet-encircling dust event observed by IR heterodyne spectroscopyv(R009-023)

        ŽRú± ~•½ (ç—t‘åŠwF‘æ2•ª–ì)
          uH-IIAƒƒPƒbƒg‘Å‚¿ã‚°‚É”º‚¤“d—£Œ—•Ï“®‚̉ðÍv(R005-26)

        ˆÉ“¡ ‹`‹N (–¼ŒÃ‰®‘åŠwF‘æ3•ª–ì)
          uComputer simulations of precipitating electrons through chorus-wave particle interactionsviR006-046j

        ˆÉŽt ‘å‹M (“Œ‹ž“s—§‘åŠwF‘æ3•ª–ì)
          u’n‹…Ž¥‹CŒ—XüŽB‘œŒv‰æ GEO-X ‚ÉŒü‚¯‚½’´Œy—ÊXü–]‰“‹¾‚̃vƒ‰ƒYƒ}Œ´Žq‘w‘ÍÏ–@‚É‚æ‚é Pt –Œ•t‰ÁHviR006-067j

        Ž›‹« ‘¾Ž÷ (“Œ‹ž‘åŠwF‘æ3•ª–ì)
          uA fluid closure in wavenumber space to model cyclotron resonance of hot magnetized plasmasviR008-016j

      R¸ˆõ

        ”©ŽR —B’Bi‰ªŽR—‰È‘åŠwF‘æ‚P•ª–ìj
        ŽR’J —S‰îiŽY‹Æ‹Zp‘‡Œ¤‹†ŠF‘æ‚P•ª–ìj
        ‘å’Ë —Yˆêi–¼ŒÃ‰®‘åŠwF‘æ2•ª–ìR005‘ã•\j
        ²“¡ ‹B•Fi‰F’ˆ‰ÈŠwŒ¤‹†ŠFF‘æ2•ª–ìR009‘ã•\j
        ’ç ‰ëŠîi‹É’nŒ¤‹†ŠF‘æ2•ª–ìj
        Ž›“c ’¼Ž÷i“Œ–k‘åŠwF‘æ2•ª–ìj
        ¼–ì ^–Øi‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ2•ª–ìj
        –ìŒû Žsi“Þ—Ç—Žq‘åŠwF‘æ2•ª–ìj
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        ŽÂŒ´ ˆçi‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ3•ª–ìR006‘ã•\j
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        ‘å–î _‘ãiç—t‘åŠwF‘æ3•ª–ìj
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        ’†‘º ³l (‰F’ˆ‰ÈŠwŒ¤‹†Š, R009‘ã•\F‘æ‚Q•ª–ì)
        Îâ Œ\Œá (•xŽRŒ§—§‘åŠwF‘æ‚Q•ª–ì)
        ¡‘º „ (“Œ‹ž‘åŠwF‘æ‚Q•ª–ì)
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        ‘å’Ë —Yˆê (–¼ŒÃ‰®‘åŠwF‘æ‚Q•ª–ì)
        ‘å–î _‘ã (ç—t‘åŠwF‘æ‚Q•ª–ì)
        ¬ì ‘×M (‘—§‹É’nŒ¤‹†ŠF‘æ‚Q•ª–ì)
        Š}‰H@N³ (“Œ–k‘åŠwF‘æ‚Q•ª–ì)
        _ŽR “O (ŽY‹Æ‹Zp‘‡Œ¤‹†ŠF‘æ‚Q•ª–ì)
        ²ì ‰p•v (‹ž“sŽY‹Æ‘åŠwF‘æ‚Q•ª–ì)
        ²“¡ Œõ‹P (–kŠC“¹‘åŠwF‘æ‚Q•ª–ì)
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        “cŒû ^ (—§‹³‘åŠwF‘æ‚Q•ª–ì)
        ’Óc ‘ì—Y (“d‹C’ÊM‘åŠwF‘æ‚Q•ª–ì)
        ¼‰ª –¢’m (î•ñ’ÊMŒ¤‹†‹@\F‘æ‚Q•ª–ì)
        Huixin Liu (‹ãB‘åŠwF‘æ‚Q•ª–ì)
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        ¼‰ª ÊŽq (‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ‚Q•ª–ì)
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        ŽRè “Ö (‰F’ˆ‰ÈŠwŒ¤‹†ŠF‘æ‚Q•ª–ì)
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        ’†a ˆ¨ (î•ñ’ÊMŒ¤‹†‹@\, R006/R010‘ã•\F‘æ‚R•ª–ì)
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        ‹gì Œ°³ (‹ãB‘åŠw, R006‘ã•\F‘æ‚R•ª–ì)
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        ‰–ì ˜a•v (–¼ŒÃ‰®‘åŠwF‘æ‚R•ª–ì)
        ¬˜H ^Žj (–¼ŒÃ‰®‘åŠwF‘æ‚R•ª–ì)
        “c’† —ǹ (‘—§‹É’nŒ¤‹†ŠF‘æ‚R•ª–ì)
        ‚‹´ Žå‰q (Johns Hopkins UniversityF‘æ‚R•ª–ì)
        Ž›–{ –œ—¢Žq (‹ãBH‹Æ‘åŠwF‘æ‚R•ª–ì)
        ¬s ‘×—T (•xŽR‘åŠwF‘æ‚R•ª–ì)
        ”\¨ ³m (–¼ŒÃ‰®‘åŠwF‘æ‚R•ª–ì)
        ‹´–{ ‹v”üŽq (‹g”õ‘Û‘åŠwF‘æ‚R•ª–ì)
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        âÀ“‡ Œh (ŠC—mŒ¤‹†ŠJ”­‹@\F‘æ‚R•ª–ì)
        ‹g‰ª ˜a•v (“Œ‹ž‘åŠwF‘æ‚R•ª–ì)

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        ‘æ‚P•ª–ì
        u’n‹…E˜f¯“à•”“dŽ¥‹CŠwi“d‹C“`“±“xA’nŠkŠˆ“®“dŽ¥‹CŠwjvAu’nŽ¥‹CEŒÃ’nŽ¥‹CEŠâÎŽ¥‹Cv
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        ²“¡ ‰ë•F (“Œ‹ž‘åŠwF‘æ‚P•ª–ì)
        ²“¡ —²—Y (–kŠC“¹î•ñ‘åŠwF‘æ‚Q•ª–ì)
        ’†ì L–± (“Œ–k‘åŠwF‘æ‚Q•ª–ì)
        ¼ŽR ®“T (‘—§‹É’nŒ¤‹†ŠF‘æ‚Q•ª–ì)
        Œj‰Ø –M—T (“Œ‹ž‘åŠwF‘æ‚R•ª–ì)
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        ­‰ª _•½ (‚’m‘åŠw: ‘æ‚P•ª–ì)
          uŽ¥«×‹Û Magnetospirillum magnetotacticum MS-1 ‚ªŠl“¾‚·‚éŽc—¯Ž¥‰»‚Æ‚»‚Ì«Ž¿‚Ì‚³‚ç‚Ȃ錟“¢v(R004-P13)

        ‘ê‘ò ‹¿Œá (“d‹C’ÊM‘åŠw: ‘æ‚Q•ª–ì)
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          u‘¾—z—zŽq~‚螂݃Cƒxƒ“ƒg‚É”º‚¤‹Éˆæ’†ŠÔŒ—ƒIƒ]ƒ“Œ¸­‚Ì“Œv‰ðÍv(R005-P35)

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        “n•Ó ‚Í‚é‚È (“Œ–k‘åŠw: ‘æ‚Q•ª–ì)
          u‚·‚΂é–]‰“‹¾‚ÅŠÏ‘ª‚³‚ꂽ–دԊOƒI[ƒƒ‰‚Ì”÷×\‘¢‚Æ‚»‚ÌŽžŠÔ•Ï“®v(R009-P16)

        àV ‹M (“Œ–k‘åŠw: ‘æ‚Q•ª–ì)
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        ¯“c @l (“Œ‹ž‘åŠw: ‘æ‚R•ª–ì)
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        “cŒû ^ (—§‹³‘åŠw, R009‘ã•\F‘æ‚Q•ª–ì)
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      ŽóÜŽÒ

        –kŒ´ —D (‹ãB‘åŠw: ‘æ‚P•ª–ì)
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      ‘æ136‰ñu‰‰‰ï (2014”N10ŒŽ31“ú-11ŒŽ3“úF¼–{)

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          uGPS-TEC‚É‚æ‚é’†ˆÜ“xƒXƒ|ƒ‰ƒfƒBƒbƒNE‚Ì‹óŠÔ\‘¢‚ÌŠÏ‘ªv(R005-35)

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          uHarmonic spectral features of upstream whistler-mode waves near the Moonv (R007-06)
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          uSub-packet structures in the EMIC triggered emission observed by the THEMIS probesv (R006-33)
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          u“ì‹Éº˜aŠî’n‚̃~ƒŠ”g•ªŒõŠÏ‘ª‚ÅŒŸo‚³‚ꂽMLT—̈æ‚ÌNO‚Ì‘‰ÁviB005-06j
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      ŽóÜŽÒ | R¸ˆõ | •ª–ìu•] | Ž––±‹Ç

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        ¼“c ˜a–çi“Œ–k‘åŠwF‘æ‚Q•ª–ìj
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