’˜ŽÒ |
”•\ŽÒ |
µ‘Ò u‰‰ |
u‰‰”Ô† |
ƒVƒ‡[ƒgƒ^ƒCƒgƒ‹ |
—\eW–{•¶ |
‰¡“c Ÿˆê˜Y |
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B006-14 |
SCOPE‰q¯“‹Ú—p“dŽqƒGƒlƒ‹ƒM[•ªÍŠí‚ÌŠJ” |
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B007-03 |
Asymmetric nightside surface charging of the Moon in the solar wind |
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# |
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B009-P009 |
‰Î¯Žü•Ó‚Å‚Ì“¯ˆÊ‘ÌŒv‘ª—pTOFŒ^Ž¿—Ê•ªÍŠí‚ÌŠJ” |
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S001-01 |
u‚©‚®‚âvMAP-PACE‚ª–¾‚ç‚©‚É‚µ‚½ŒŽ’‹ŠÔ‘¤‚ÌŒŽ\‘¾—z•—‘ŠŒÝì—p |
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S001-02 |
Solar wind proton access deep into the near-Moon wake observed by SELENE (KAGUYA) |
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# |
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S001-04 |
ŒŽŽ¥‹CˆÙí‚É‚æ‚錎–Ê‚Å”½ŽË‚³‚ꂽ‘¾—z•—ƒCƒIƒ“‚̉Á‘¬ |
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S001-07 |
ŒŽŽü‰ñ‰q¯u‚©‚®‚âv“‹Ú“dŽq•ªÍŠíMAP-PACE-ESA‚ð—p‚¢‚½ŒŽŽ¥‹CˆÙíŠÏ‘ª |
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S001-08 |
‚©‚®‚â‰q¯ŠÏ‘ª‚Ɋvƒ‰ƒYƒ}ƒV[ƒg“dŽq‚ÆŒŽ–Ê‚Ì‘ŠŒÝì—p‚ÌŒ¤‹† |
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S001-12 |
ŒŽŽü•ÓƒCƒIƒ“ŠÏ‘ª‚ÆŒŽŠó”–‘å‹C‚Ì\‘¢ |
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S001-P008 |
Solar wind ion reflection by lunar magnetic anomalies |
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S001-P009 |
‚©‚®‚â‚É‚æ‚邃Gƒlƒ‹ƒM[ŒŽ•\–Ê”½ŽË‰Á‘¬ƒCƒIƒ“‚ÌŠÏ‘ª |
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S001-P010 |
‘¾—z•—ƒvƒƒgƒ“‚ÌŒŽ–ÊŽU—‚É‚¨‚¯‚é•ûŒüˆË‘¶«‚ÌŒ¤‹† |
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S001-P011 |
‚©‚®‚â‰q¯ƒf[ƒ^‚ð—p‚¢‚½ƒTƒuƒXƒg[ƒ€Žž‚ÌŽ¥‹CŒ—”ö•”‚‘¬ƒvƒ‰ƒYƒ}—¬‚ÌŒ¤‹† |
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‰¡ŽR —³G |
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B005-27 |
Ô“¹‘å‹CƒŒ[ƒ_[‚Å’‹ŠÔ‚ÉŠÏ‘ª‚³‚ꂽ‚“x150km‰ˆŽ¥—Íü•s‹K‘¥\‘¢‚Ì“Œv‰ðÍ |
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‰¡ŽR —Y¶ |
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B005-13 |
DELTA-2ƒLƒƒƒ“ƒy[ƒ“TMA‚É‚æ‚éƒI[ƒƒ‰”¶Žž‚Ì”MŒ—‰º•”’†«•—‚Ì‚¸“x‰ðÍ |
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B005-28 |
WINDƒƒPƒbƒgŽÀŒ±‚É‚¨‚¯‚éLi•úo—Ê‚¨‚æ‚Ñ”ŒõŠñ—^—¦‚Ì„’è |
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‰¡ŽR —S“T |
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A004-10 |
Ž÷–Ø”N—Ö’†‚Ì•úŽË«’Y‘f”Z“x•ªÍ‚É‚æ‚鑾—zŠˆ“®‚¨‚æ‚Ñ’nŽ¥‹C•Ï“®‚Ì•œŒ³‚ɂ‚¢‚Ä |
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A004-P012 |
Be-10ƒtƒ‰ƒbƒNƒX•Ï“®‚ÉŠî‚ÂPaleomagnetic lock-in depth‚ÌŒˆ’è |
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B010-24 |
Ž÷–Ø”N—Ö’†‚Ì•úŽË«’Y‘f”Z“x‚É‚à‚Ƃ‘¾—zŠˆ“®‹É¬Šú‚Ì‘O’›Œ»Û‚ɂ‚¢‚Ä |
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‰¡ŽR —R‹IŽq |
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A004-P006 |
’nŽ¥‹C‰i”N•Ï‰»Fu•½‹Ïv‚Æu•Ï‰»v‚Ì‹« |
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A004-P007 |
“ú–{‚É‚¨‚¯‚élŒÃ’nŽ¥‹CŠwƒf[ƒ^‚©‚ç‚̉i”N•Ï‰»‹Èü‚Ìì¬ |
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‹g‰ª ˜a•v |
# |
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B009-P005 |
The EUV spectroscopic observation of Io plasma torus |
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B009-P014 |
Master the method to increase quantum efficiency of a microchannel plate (MCP) |
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‹gì Œ°³ |
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B005-38 |
Analytic representation for quiet daily geomagnetic variations |
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B006-29 |
Phase Relation of the Ionospheric Doppler Velocity and Magnetic Pi 2 Pulsations |
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B006-32 |
A detection of substorm precursors by SSA-based change-point analysis |
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B006-P017 |
Automatic Identification of Pi 2 using MAGDAS/CPMN -Toward Construction of a new Pi 2 Index- |
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B006-P018 |
An application of frequency-domain ICA to Pi 2 pulsations |
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B006-P020 |
A new interpretation of high-latitude Pi 2 observed at the MAGDAS/CPMN stations |
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* |
B009-12 |
”’lŒvŽZƒvƒƒWƒFƒNƒg‚Ì«—ˆ‘œ‚Ƙf¯“dŽ¥Œ—‚Ì—‰ð‚Ì¡Œã |
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# |
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B010-03 |
Ž¥‹CŒ—“d—£Œ—Œ‹‡“d—¬Œn‚̕“I‹Lq‚Æ—‰ð |
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B010-P003 |
ƒAƒ‹ƒtƒFƒ“”g‚ð‰îÝ‚µ‚½ƒI[ƒƒ‰‘Ñ‚ÌŽ¥‹CŒ—“d—£Œ—Œ‹‡ |
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B010-P014 |
ULTIMA Magnetic Power Spectral Density and its Radial Diffusion Coefficients for REE |
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‹gì ˆê˜N |
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B006-27 |
Observation of Plasmaspheric Refilling using Cross-Phase Measurements |
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B006-P035 |
ƒvƒ‰ƒYƒ}Œ—ŠO‘¤‹«ŠEˆæ‚ÉŒ©‚ç‚ê‚éshoulder\‘¢‚̶¬‰ß’ö‚ÌÄl |
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B006-P037 |
notch‚ÌŒ`¬ƒƒJƒjƒYƒ€‚ƃvƒ‰ƒYƒ}Œ—‚̉ñ“]‘¬“x |
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B009-P005 |
The EUV spectroscopic observation of Io plasma torus |
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B009-P014 |
Master the method to increase quantum efficiency of a microchannel plate (MCP) |
•\Ž¦ |
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B010-06 |
ISS-IMAPƒ~ƒbƒVƒ‡ƒ“‚Æ‚»‚̉F’ˆ“V‹CŒ¤‹†‚Ö‚Ì—˜—p |
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# |
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S001-09 |
‹É’[Ž‡ŠOŒõ–]‰“‹¾‚ÌŽc‚µ‚½¬‰Ê |
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S001-P012 |
RESONANCE EMISSION OF OXYGEN IONS IN THE TERRESTRIAL POLAR WIND (2) |
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S001-P014 |
Identifying the Plasmapause Using Ground-based Magnetometers, IMAGE-EUV, and KAGUYA-TEX Data |
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‹gì ^“o |
# |
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B006-P027 |
“à•”Ž¥‹CŒ—‚É‚¨‚¯‚éƒzƒCƒbƒXƒ‰[ƒ‚[ƒhEƒR[ƒ‰ƒX”g‚É‚æ‚éƒTƒCƒNƒƒgƒƒ“‹¤–“dŽq‰Á‘¬ |
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‹g“c Œ’Œå |
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B005-13 |
DELTA-2ƒLƒƒƒ“ƒy[ƒ“TMA‚É‚æ‚éƒI[ƒƒ‰”¶Žž‚Ì”MŒ—‰º•”’†«•—‚Ì‚¸“x‰ðÍ |
•\Ž¦ |
# |
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B005-24 |
TARANIS ‰q¯‹y‚Ñ JEM-GLIMS ‚É“‹Ú‚·‚éƒtƒHƒgƒ[ƒ^‚ÌŠJ” |
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‹g“c ˜aÆ |
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B005-24 |
TARANIS ‰q¯‹y‚Ñ JEM-GLIMS ‚É“‹Ú‚·‚éƒtƒHƒgƒ[ƒ^‚ÌŠJ” |
•\Ž¦ |
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B005-P011 |
GLIMS Mission: Optical and Electromagnetic Observation of Lightning and TLEs from ISS |
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B009-P010 |
Balloon-Borne Telescope System for Optical Remote Sensing of Planetary Atmospheres and Plasmas |
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‹g“c ‘å‹I |
# |
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B010-P009 |
Data visualization for space weather/climate study using data-showcase system, Dagik |
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‹g“c ’¼l |
# |
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B005-P033 |
’´’á‹O“¹‰q¯‚É‚æ‚é”M‘Ñ‘å‹Cï—‚ÌGPS‰†•ÁŠÏ‘ª‚Ì’ñˆÄ |
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‹g“c ‰pl |
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B005-P007 |
MUƒŒ[ƒ_[25chŠ±ÂŒv‚É‚æ‚é‚Ó‚½‚²ŒQƒwƒbƒhƒGƒR[ŠÏ‘ª‚Ì“Œv“I•]‰¿ |
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‹gŒ´ V |
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A004-P007 |
“ú–{‚É‚¨‚¯‚élŒÃ’nŽ¥‹CŠwƒf[ƒ^‚©‚ç‚̉i”N•Ï‰»‹Èü‚Ìì¬ |
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‹g‘º ~ |
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B009-P010 |
Balloon-Borne Telescope System for Optical Remote Sensing of Planetary Atmospheres and Plasmas |
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‹g‘º —ߌd |
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A003-P004 |
VŠƒ|_ŒË‚Ђ¸‚ÝW’†‘Ñ‚É‚¨‚¯‚éLˆæ“I‚È”ä’ïR\‘¢ |
•\Ž¦ |
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A003-P005 |
’†•”“ú–{VŠƒ-_ŒË˜c‚ÝW’†‘ÑŽü•Ó‚̃lƒbƒgƒ[ƒNMTŠÏ‘ª (1) |
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A003-P007 |
ŽR‰A’n•û‚Ŏ擾‚³‚ꂽŠCˆæE—¤ˆæƒf[ƒ^‚ð—p‚¢‚½ŽR‰A’n•û‚Ì”ä’ïR\‘¢ |
•\Ž¦ |
# |
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A003-P009 |
Shallow resistivity structure around earthquake swarm area deduced from dense AMT/MT observations |
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‹g‘º —æŽq |
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B005-P037 |
Suppression mechanisms of PRE related with the pre-sunset CEJ |
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•Ä“c ¶ |
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B009-06 |
Simulation of water group neutral density in Saturn's inner magnetosphere |
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# |
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B009-P006 |
ƒCƒI‰ÎŽRŠˆ“®‚Ì’†ŠÔÔŠOüŠÄŽ‹ŠÏ‘ªŒv‰æ |
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