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ƒVƒ‡[ƒgƒ^ƒCƒgƒ‹ |
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ƒfƒBƒo@ƒfƒBƒGƒm |
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R003-09 |
Electrical resistivity structure beneath the southern part of Tohoku, NE Japan, revealed by magnetotelluric (MT) survey |
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o‘º@—T‰p |
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R009-33 |
ƒŠƒ€ŠÏ‘ª‚É‚æ‚é‰Î¯‘å‹C‰”’¼\‘¢‚̉𖾂ð–ÚŽw‚·V‘å‹CƒŠƒgƒŠ[ƒoƒ‹‹Zp‚ÌŒŸØ |
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Ž›‘ò@•q•v |
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R007-03 |
‚©‚Ƀpƒ‹ƒT[‚Ì‹‘å“d”gƒpƒ‹ƒX‚ð—p‚¢‚½ƒTƒCƒNƒ‹24/25‹É¬Šú‚É‚¨‚¯‚鑾—zƒRƒƒi–§“x‘ª’è |
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Ž›“c@ˆê¶ |
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R005-25 |
COSMIC-2‰q¯“‹Ú‚QŽü”gƒr[ƒRƒ“ŠÏ‘ª‚É‚æ‚é“Œ“ìƒAƒWƒAˆæ‚̃vƒ‰ƒYƒ}ƒoƒuƒ‹‚ÉŒq‚ª‚肤‚é“d—£Œ—‚Ì’·”g’·•Ï“®‚ÉŠÖ‚·‚錤‹† |
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Ž›“c@D |
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R005-38 |
‰Î¯”MŒ—“d—£Œ—‚É‚Ý‚ç‚ê‚é–§“xï—‚Ì—ã‹NŒ¹ |
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Ž›“c@’¼Ž÷ |
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R005-38 |
‰Î¯”MŒ—“d—£Œ—‚É‚Ý‚ç‚ê‚é–§“xï—‚Ì—ã‹NŒ¹ |
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R006-08 |
u‚·‚´‚v‚Æ XMM-Newton ‰q¯‚É‚æ‚é’n‹…Žü•Ó“d‰×ŒðŠ·Xü‚Ì‘½“_“¯ŽžŠÏ‘ª |
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R007-10 |
u‚Ђ³‚«v‰q¯‚É‚æ‚é˜f¯ŠÔ‹óŠÔ‚̃wƒŠƒEƒ€ŒõŠwŠÏ‘ª |
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R008-07 |
A new global multifluid MHD model with the cubed sphere focusing on Martian ionosphere and magnetosphere |
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R009-06 |
‘¾—zŒn“V‘̂̉F’ˆ•—‰»ÄŒ»ŽÀŒ±‚ÉŒü‚¯‚½”Ä—pƒvƒ‰ƒYƒ}ÆŽË‘•’u‚ÌŠJ”E•]‰¿‚ÌŒ»ó |
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R009-15 |
‚ƒRƒ“ƒgƒ‰ƒXƒg–]‰“‹¾PLANETS‚ÌŠJ”󋵂Ƙf¯E‰q¯‹ß–T‚ÌŠó”–ƒKƒX”Œõ‚ÌŒŸo‰Â”\« |
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R009-17 |
ŒnŠO˜f¯‚‘w‘å‹CŠÏ‘ª‚ÉŒü‚¯‚½‘ÛŽ‡ŠOü“V•¶‰q¯WSO-UVŒv‰æ‚Ìó‹µ |
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R009-21 |
A technique for retrieving the Martian hot oxygen exosphere from O+ pickup ion measurements in the magnetosheath |
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R009-22 |
MAVEN‚¨‚æ‚ÑMars Express‚É‚æ‚é‰Î¯“d—£Œ—•s‹K‘¥\‘¢‚̉“ŠuE’¼Ú“¯ŽžŠÏ‘ª |
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R009-23 |
On plasmasphere formation around terrestrial exoplanets: Possible evidence of exoplanetary intrinsic magnetic field and atmosphere |
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R009-24 |
Numerical experiments of exospheric retrieval for isotope ratio measurements by MSA onboard MMX |
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R009-25 |
Development of an engineering model (EM) of the Mass spectrum Analyzer (MSA) for Mars Moons eXploration (MMX) |
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R009-26 |
TGO/NOMAD‚©‚烊ƒgƒŠ[ƒoƒ‹‚µ‚½‰Î¯’†ŠÔŒ—E‰º•””MŒ—‚ÌCO/CO2•ª•z‚Ì•Ï“® |
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R009-27 |
CO2‹ßÔŠO‹zŽû‚ƉQŠgŽU‹“x‚É‚æ‚é‰Î¯”MŒ—\‘¢‚ւ̉e‹¿ |
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R009-29 |
‘¾—z‚ƒGƒlƒ‹ƒM[—±Žq‚ª‰Î¯ƒIƒ]ƒ“‚É—^‚¦‚é‰e‹¿‚Ì•]‰¿ |
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R009-31 |
Numerical prediction of changes in atmospheric compositions during SEP events at Mars |
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R009-42 |
Longitudinal variation in the Venusian cloud optical thickness associated with a Kelvin wave |
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S001-10 |
2030”N‘ã‚ðŒ©˜‚¦‚½’n‹…Œ^˜f¯Œ—ŠÂ‹«Œ¤‹†‚Ì«—ˆ\‘z |
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S001-12 |
SGEPSS«—ˆ‰q¯Œv‰æƒ[ƒhƒ}ƒbƒvô’èƒ^ƒXƒNƒ`[ƒ€‚É‚¨‚¯‚éSTP‰q¯’T¸Œv‰æŒŸ“¢ |
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# |
* |
S001-16 |
“ú–{˜f¯‰ÈŠw‰ï‚Ì«—ˆ\‘z‹c˜_ |
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Ž›–{@–œ—¢Žq |
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R006-10 |
Field-aligned low-energy O+ (FALEO) ion flux enhancements in the inner magnetosphere: A possible source of warm plasma cloak |
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R006-11 |
Contribution of magnetospheric pressure inhomogeneities to SAPS Wave Structures: Arase and SuperDARN conjugated observations |
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R006-13 |
second harmonic poloidal ULF”g“®‚É‚æ‚郊ƒ“ƒOƒJƒŒƒ“ƒg—zŽq‚Ì“®Œa—A‘—F‚ ‚点ERBSP-B‰q¯‚ÌŠÏ‘ª |
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R006-15 |
A statistical survey of Pc5 waves observed in the dusk and night sectors |
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R006-24 |
Possible observation plans for high-energy analyzer (PINO) onboard a CubeSat (BIRDS-5) |
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R006-50 |
A new calibration method for LEPe low-energy electron data of the ERG satellite |
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R006-64 |
ULF modulation of the D-region ionosphere observed by VLF/LF transmitter signals |
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R010-24 |
Feasibility Study of Space Weather Observation by CubeSat in LEO |
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Ɖ®@‹M‘å |
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R008-09 |
ƒtƒB[ƒhƒoƒbƒN•sˆÀ’è«‚Ì”ñüŒ`”“W‚É‚¨‚¯‚鎞‹óŠÔ\‘¢ |
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“c@Œõ] |
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R010-25 |
NICT‰F’ˆ“V‹C—\•ñ‚Ì’†’·ŠúŒv‰æ‚Æ«—ˆ\‘z |
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