@’˜ŽÒ@ |
”•\ŽÒ |
µ‘Ò u‰‰ |
u‰‰”Ô† |
ƒVƒ‡[ƒgƒ^ƒCƒgƒ‹ |
@—\e@ |
‚“‡@ƒ^ƒPƒV |
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R006-P19 |
ERG/Arase‰q¯‚ð—p‚¢‚½‚ƒGƒlƒ‹ƒM[“dŽq‚̃sƒbƒ`Šp•ª•z‚Ì’²¸
ƒf[ƒ^ |
•\Ž¦ |
š¹@çq |
# |
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R005-P22 |
GAIA‹Éˆæ•Ï“®”Å‚ð—p‚¢‚½‘å‹K–ÍŽ¥‹C—’’†‚ÌNmF2‚ÆTEC‚̈قȂéU•‘‚Ì’²¸ |
•\Ž¦ |
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R009-33 |
LAPYUTAŒv‰æ(˜f¯‰ÈŠwA¶–½Œ—‰ÈŠwA‚¨‚æ‚Ñ“V•¶Šw‚ÉŒü‚¯‚½Ž‡ŠOü‰F’ˆ–]‰“‹¾)‚ÌŒŸ“¢ó‹µ |
•\Ž¦ |
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R010-11 |
Reproduction of electron density variation in the ionospheric D region during solar flares by the PHITS and GAIA models |
•\Ž¦ |
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R010-13 |
SOLAR-C/SoSpIM‚ªŠÏ‘ª‚·‚鑾—z•úŽË‚Ì’n‹…ã‘w‘å‹C‚ւ̉e‹¿ |
•\Ž¦ |
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R010-P10 |
ƒ‚ƒfƒ‹ƒpƒ‰ƒƒ^“™‚É‚æ‚é‘å‹CE“d—£Œ—ƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“‚Ì•sŠm’è«‚Ì•]‰¿ |
•\Ž¦ |
# |
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R011-11 |
GAIAƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“ƒf[ƒ^‚ÌIUGONETEDOI“o˜^‚ÉŒü‚¯‚Ä\DOI“o˜^ƒVƒXƒeƒ€‚ÌXVŒv‰æ |
•\Ž¦ |
“c”ö@—Á |
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R006-18 |
A two?stage deflection system for the extension of the energy coverage in space plasma three?dimensional measurements |
•\Ž¦ |
‚–Ø@¹Žq |
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R009-13 |
‹ßÔŠOŽB‘œ‘•’uTOPICSŠJ”‚Æ–¼ŠñƒsƒŠƒJ–]‰“‹¾‚ł̃tƒ@[ƒXƒgƒ‰ƒCƒg |
•\Ž¦ |
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R009-19 |
‚Ђ³‚«‰q¯ŠÏ‘ªŒ‹‰Ê‚Æ”äŠr‚µ‚½ƒWƒIƒRƒƒiƒ‚ƒfƒ‹‚̑Ó–«‚ÌŒŸØ |
•\Ž¦ |
# |
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R009-P08 |
ƒGƒEƒƒp‘å‹C‚É‚¨‚¯‚锌õ‹Pü‚Ì’TõF’nã–]‰“‹¾‚É‚æ‚é‰ÂŽ‹ŠÏ‘ª |
•\Ž¦ |
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R009-P09 |
˜f¯‚•ªŽUƒGƒVƒFƒ‹•ªŒõŠíESPRIT‚ÌŠJ”‚Æ‹ßÔŠOŽB‘œ‘•’uTOPICS‚̉ŠúŠÏ‘ª•ñ |
•\Ž¦ |
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R009-P12 |
–]‰“‹¾ŠÏ‘ª‚ð—p‚¢‚½“V‰¤¯‘å‹C‚Ì—A‘—‘¬“x‚Ì„’è |
•\Ž¦ |
‚–Ø@ªO |
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R009-P26 |
“d”g‰†•Á–@‚ð—p‚¢‚½‹à¯Ô“¹ˆæ‚É‚¨‚¯‚é”M’ªŽ¬”g‚̉”’¼\‘¢‚ÉŠÖ‚·‚éŠÏ‘ª“IŒ¤‹† |
•\Ž¦ |
‚‘q@Lˆê |
# |
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R003-01 |
‹à‘®z•¨’T¸‚Ì‚½‚ß‚ÌŠâΓd‹C•¨«‚Ì‘ª’è‚ƃf[ƒ^ƒx[ƒX‰» |
•\Ž¦ |
‚“‡@Œ’ |
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R006-05 |
–¬“®ƒI[ƒƒ‰‚É”º‚¤•L‚¢ƒGƒlƒ‹ƒM[‘Ñ‚Ì“dŽq‚Ì~‚肱‚ÝF‚ ‚点‰q¯-EISCAT‚Ì‹¤“¯ŠÏ‘ª‹y‚уVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“ |
•\Ž¦ |
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R006-19 |
New method for calibrating Arase HEP-L data using XEP data and Geant4 simulation of MeV electron contamination |
•\Ž¦ |
‚“‡@Œ’ |
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R010-22 |
•úŽËü‘ÑŠO‘Ñ“dŽq•Ï“®—\‘ªƒ‚ƒfƒ‹‚ÌŠJ”‚ÆXAI‚É‚æ‚郂ƒfƒ‹‰ðŽß |
•\Ž¦ |
‚“c@‰ëN |
# |
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R005-15 |
Properties of ionospheric low-altitude ion upflows during CIR- and CME- driven magnetic storms based on the EISCAT observations |
•\Ž¦ |
‚–ì@Œü—z |
# |
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R006-P02 |
Ž¥‹C—’’†‚É”¶‚µ‚½ƒIƒƒKƒoƒ“ƒhƒI[ƒƒ‰‚É”º‚¤•úŽËü‘Ñ“dŽq~‰º‚ÌŽž‹óŠÔ•Ï“®: ‘½Žü”gƒŠƒIƒ[ƒ^CEMCCD ‘S“VƒJƒƒ‰‚É‚æ‚铯ŽžŠÏ‘ª |
•\Ž¦ |
‚‹´@ˆê˜Y |
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R011-15 |
Œ¤‹†ƒf[ƒ^‚ð‚æ‚茩‚‚¯‚â‚·‚‚·‚邽‚߂̃ƒ^ƒf[ƒ^•ÏŠ·‚Æ‹@ŠÖƒŠƒ|ƒWƒgƒŠ‚Ö‚Ì“o˜^ |
•\Ž¦ |
‚‹´@Œc‘¾˜Y |
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R009-P06 |
ŒŽ–Ê“V•¶‘äFƒ[ƒgƒ‹”g“d”gŠ±ÂŒv‚ÌŠT”OŒŸ“¢ |
•\Ž¦ |
‚‹´@“§ |
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R005-02 |
Es‘wŒ`¬‰ß’ö‚Ì’†«‘å‹C‚ƃvƒ‰ƒYƒ}‘å‹C‚Ì“¯ŽžŠÏ‘ª‚É‚æ‚é‰ð–¾: RIDEƒLƒƒƒ“ƒy[ƒ“ |
•\Ž¦ |
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R005-20 |
S-520-27†‹@ŠÏ‘ªƒƒPƒbƒg‚É‚æ‚é–éŠÔ’†‹K–Í“`”À«“d—£Œ—ï—”¶Žž‚Ì“dêŠÏ‘ªŒ‹‰Ê |
•\Ž¦ |
# |
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R005-21 |
Tomographic imaging of sporadic E-layer by sounding rocket S-520-32 observation |
•\Ž¦ |
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R005-24 |
q‹óq–@—p“d”gILS Localizer‚ð—p‚¢‚½ƒXƒ|ƒ‰ƒfƒBƒbƒN E ‘w‹óŠÔ\‘¢‚̉ðÍ |
•\Ž¦ |
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R005-31 |
Strong ionospheric irregularities in sunlit conditions and its impact on GNSS-based navigation systems |
•\Ž¦ |
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R005-P03 |
Naƒ‰ƒCƒ_[‚Ì’‹ŠÔŠÏ‘ª‚É—p‚¢‚éFaraday filter‚Ì“§‰ß—¦Úבª’è |
•\Ž¦ |
‚‹´@’¼Žq |
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R006-36 |
Excitation of internally driven ULF waves of a weakly magnetized planet based on the magnetosphere-ionosphere coupled model |
•\Ž¦ |
# |
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R006-P14 |
Examination of method to separate noise from natural magnetic field measured on geostationary satellite |
•\Ž¦ |
# |
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R010-14 |
Forecast of Geomagnetic Field Disturbances Using the Empirical Model for Space Weather |
•\Ž¦ |
‚‹´@‘¾ |
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R004-01 |
Strong magnetic anomalies record the weak dynamo field of ancient Mars |
•\Ž¦ |
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R004-02 |
˜f¯ƒ_ƒCƒiƒ‚ŒvŽZ‚ÉŠî‚Â…¯Lowes”¼Œa‚ƃ_ƒCƒiƒ‚”¼Œa‚Ì”äŠr |
•\Ž¦ |
# |
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R004-P01 |
Numerical study of dynamo action generating equatorially asymmetric magnetic fields |
•\Ž¦ |
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R009-05 |
Ž¥‹CŒ—ƒ[ƒu‚É‚¨‚¯‚é’‹‘¤ŒŽ–Ê“dˆÊ‚̃}ƒbƒsƒ“ƒO‚ÉŒü‚¯‚½‚©‚®‚â‚ÆARTEMISŠÏ‘ª‚ð—p‚¢‚½‰Šú‰ðÍ |
•\Ž¦ |
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R009-P05 |
‚©‚®‚â’á‚“xŠÏ‘ªƒf[ƒ^‚ð—p‚¢‚½ŒŽƒ~ƒjŽ¥‹CŒ—‚̉דd—±ŽqE“dŽ¥ê“Á«‚ÌŒ¤‹† |
•\Ž¦ |
‚‹´@KO |
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R009-P12 |
–]‰“‹¾ŠÏ‘ª‚ð—p‚¢‚½“V‰¤¯‘å‹C‚Ì—A‘—‘¬“x‚Ì„’è |
•\Ž¦ |
ûüŒ´@—ž”T |
# |
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R006-P18 |
‚ ‚点‰q¯‚ÅŠÏ‘ª‚³‚ꂽ~‚èž‚Ý“dŽq‚Ì“Œv“I‰ðÍ |
•\Ž¦ |
‚‘º@–¯—Y |
|
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R005-35 |
Variations in the D-region ionosphere after the 2022 Tonga volcanic eruption using AVON VLF/LF transmitter signals |
•\Ž¦ |
‚ŽR@‹v”ü |
# |
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R005-28 |
”¼‹…ŠÔ‰ˆŽ¥—Íü“d—¬iIHFACj‚ÉŒ»‚ê‚适U“ú”g‚Ì•Ï“® |
•\Ž¦ |
“cì@‰ël |
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|
R005-02 |
Es‘wŒ`¬‰ß’ö‚Ì’†«‘å‹C‚ƃvƒ‰ƒYƒ}‘å‹C‚Ì“¯ŽžŠÏ‘ª‚É‚æ‚é‰ð–¾: RIDEƒLƒƒƒ“ƒy[ƒ“ |
•\Ž¦ |
‘ê@•üŒb |
# |
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R006-P20 |
Estimation of low-energy electron temperature using Arase satellite interferometry observations |
•\Ž¦ |
“cŒû@‘ |
|
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R005-36 |
ƒgƒ“ƒKŠC’ê‰ÎŽR•¬‰Î‚É‚æ‚蔶E“`”À‚µ‚½Lamb”g‚ٕ̈û«‚Æ“d—£Œ—“dŽq–§“xï—•ª•zˆÙ•û«‚ÌŠÖŒW |
•\Ž¦ |
|
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R006-06 |
Intense low-energy electron precipitation associated with poleward expansion of red auroras near the nightside polar cap boundary |
•\Ž¦ |
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R006-13 |
Outflow jets from lobe reconnection: Roles of shear flow in reconnection |
•\Ž¦ |
# |
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R006-25 |
Alfvenic features at 500 km altitude for the cusp aurora |
•\Ž¦ |
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R008-05 |
’áˆæ¬¬”g‚’²”g‚Ì—ã‹N‚¨‚æ‚Ñ”ñüŒ`”“W‚ÉŠÖ‚·‚éƒpƒ‰ƒ[ƒ^[ˆË‘¶« |
•\Ž¦ |
“cŒû@^ |
|
|
R009-07 |
œa¯ƒRƒ}’†‚ÌD/HŠÏ‘ª‚ð–Ú“I‚Æ‚µ‚½‹¤–‹zŽûŒ^ƒtƒBƒ‹ƒ^‚ÌŠJ” |
•\Ž¦ |
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R009-30 |
LIR‚Ì’·ŠúŠÏ‘ª‚©‚瓾‚ç‚ꂽ‹à¯‰_ã‘w‚Å‚Ì•½‹Ï‰·“x‚Æ”M’ªŽ¬”g‚Ì•Ï“® |
•\Ž¦ |
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R009-31 |
Characteristics of Venusian gravity waves inferred from thermal infrared cloud images |
•\Ž¦ |
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R009-P25 |
Image analysis of the polar vortices of Venus observed by Akatsuki/LIR |
•\Ž¦ |
’|“à@’¼”V |
# |
|
R009-P21 |
•¡”’T¸‹@ŠÏ‘ª‚ÉŠî‚”ö•”ƒCƒIƒ“ŽUˆí‚Ì‹Ÿ‹‹Œ¹‚ÌŒ¤‹† |
•\Ž¦ |
’|è@‘¾’q |
|
|
R008-P03 |
1ŽŸŒ³PICŒvŽZ‚É‚æ‚é‘åŒ^ƒŒ[ƒU[ŽÀŒ±‚É‚¨‚¯‚é–³Õ“ËÕŒ‚”g¶¬‹@\‚̉𖾠|
•\Ž¦ |
’|Œ´@‘å’q |
# |
|
R007-P02 |
FPGA ‚ð—p‚¢‚½‘¾—zŠÏ‘ª—p“d”g–]‰“‹¾‚ÌŠJ” |
•\Ž¦ |
’|L@^ˆê |
|
|
R009-25 |
‚‘¬‰ñ“]‹…Šk“à‚Ì”ñ’e«—¬‘Ì‚Ì”M‘Η¬‚Ì’·ŽžŠÔÏ•ª |
•\Ž¦ |
Šx“¡@ˆêG |
|
|
R009-P01 |
”ÑŠÚE‘ ‰¤ŠÏ‘ªŠ‚ð—p‚¢‚½’áŽü”gVLBIŽÀŒ± |
•\Ž¦ |
é@„Šó |
# |
|
R006-P25 |
Effects of ULF oscillation on the duct propagation of whistler-mode chorus emissions |
•\Ž¦ |
’F@DK |
|
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R003-10 |
‹SŠEƒJƒ‹ƒfƒ‰‰ÎŽRŠC’ꉺ‚ÌŽOŽŸŒ³”ä’ïR\‘¢‰ðÍ |
•\Ž¦ |
—§¼@rˆê |
|
|
R006-21 |
Low-cost magnetometers using MI sensors: Estimation of magnetospheric plasma mass density from multi-point observation |
•\Ž¦ |
“c’†@ŠG”ü |
# |
|
R009-P04 |
Kaguya/LRS‚̃I[ƒƒ‰ƒLƒƒ[ƒ^•úŽËŠÏ‘ª‚ð—p‚¢‚½ƒpƒbƒVƒuƒŒ[ƒ_[‚É‚æ‚錎–Ê‹y‚Ñ’n‰º\‘¢’T¸Žè–@‚ÌŒŸ“¢ |
•\Ž¦ |
“c’†@FŽ¡ |
|
|
R005-03 |
Development of 1U-size impedance probe for cube satellite missions |
•\Ž¦ |
“c’†@Žü‘¾ |
|
|
R008-P03 |
1ŽŸŒ³PICŒvŽZ‚É‚æ‚é‘åŒ^ƒŒ[ƒU[ŽÀŒ±‚É‚¨‚¯‚é–³Õ“ËÕŒ‚”g¶¬‹@\‚̉𖾠|
•\Ž¦ |
“c’†@½Žu˜Y |
|
|
R006-17 |
A New Technique for Space Plasma Measurements Using Floating-mode Avalanche Photodiode Combined with Electrostatic Energy Analyzer |
•\Ž¦ |
“c’†@‚Žj |
|
|
R006-09 |
‰ˆŽ¥—Íü“d—¬ƒ_ƒCƒiƒ‚‚Æ’nŽ¥‹CƒTƒuƒXƒg[ƒ€”’B‚ÌŠÖŒW‚ɂ‚¢‚Ä |
•\Ž¦ |
|
|
R006-10 |
–kŒü‚«IMF‚Å‚ÌŽ¥‹CŒ—“d—£Œ—‘Η¬‚Ænull-separator\‘¢ |
•\Ž¦ |
|
|
R006-11 |
‹ÉŠ¥•ªŠò‚ÌŽ¥êƒgƒ|ƒƒW[ |
•\Ž¦ |
|
|
R006-12 |
Scattered perpendicular flow speed in the dayside reconnection regions due to change in the IMF Bz direction |
•\Ž¦ |
|
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R006-15 |
ƒTƒuƒXƒg[ƒ€Žž‚Ì’n‹…‹ß–Tƒvƒ‰ƒYƒ}ƒV[ƒg‚É‚¨‚¯‚éƒCƒIƒ“‚̉Á‘¬—¦‚̃Gƒlƒ‹ƒM[Aƒsƒbƒ`ŠpAŽ¿—ÊA“d‰×ˆË‘¶« |
•\Ž¦ |
|
|
R006-23 |
Evolution of M-I convection depending on the Alfven conductance as simulated by global MHD model with Alfvenic coupling |
•\Ž¦ |
|
|
R009-18 |
Effects of stellar XUV spectra on atmospheric escape from a Mars-like planet orbiting inactive low-mass stars |
•\Ž¦ |
|
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R010-21 |
Nighttime geomagnetic response to jumps of solar wind dynamic pressure:
A possible cause of Quebec blackout in March 1989 |
•\Ž¦ |
“c’†@—FŒ[ |
# |
|
R005-P10 |
ELFIN‰q¯‚ÆEISCATƒŒ[ƒ_[‚ÌŠÏ‘ªŒ‹‰Ê‚ð—p‚¢‚Ä‰ð‚«–¾‚©‚·~‚èž‚Ý“dŽq‚É‚Í‚½‚炃~ƒ‰[—Í‚ª“dŽq–§“x‚Ì‚“x•ª•z‚É—^‚¦‚éŒø‰Ê |
•\Ž¦ |
“c’†@^ |
|
|
R005-04 |
ŠÏ‘ªƒƒPƒbƒg“‹Ú’´‚‘w‘å‹CŠÏ‘ª—p^‹óŒv‚ÉŠÖ‚·‚錤‹† |
•\Ž¦ |
|
|
R005-20 |
S-520-27†‹@ŠÏ‘ªƒƒPƒbƒg‚É‚æ‚é–éŠÔ’†‹K–Í“`”À«“d—£Œ—ï—”¶Žž‚Ì“dêŠÏ‘ªŒ‹‰Ê |
•\Ž¦ |
|
|
R005-P11 |
Analysis of plasma waves observed by LFAS/WFC onboard the SS-520-3 sounding rocket |
•\Ž¦ |
“c’†@‰ëb |
|
|
R009-33 |
LAPYUTAŒv‰æ(˜f¯‰ÈŠwA¶–½Œ—‰ÈŠwA‚¨‚æ‚Ñ“V•¶Šw‚ÉŒü‚¯‚½Ž‡ŠOü‰F’ˆ–]‰“‹¾)‚ÌŒŸ“¢ó‹µ |
•\Ž¦ |
“c’†@—Bˆí |
|
|
R008-P11 |
ƒR[ƒhŠÔŒ‹‡ƒtƒŒ[ƒ€ƒ[ƒN‚ɊF’ˆŠÂ‹«•Ï“®|‰q¯‘Ñ“dŒ»Û˜A¬‰ð̓vƒ‰ƒbƒgƒtƒH[ƒ€‚ÌŠJ” |
•\Ž¦ |
“c’†@—ǘa |
|
|
R005-36 |
ƒgƒ“ƒKŠC’ê‰ÎŽR•¬‰Î‚É‚æ‚蔶E“`”À‚µ‚½Lamb”g‚ٕ̈û«‚Æ“d—£Œ—“dŽq–§“xï—•ª•zˆÙ•û«‚ÌŠÖŒW |
•\Ž¦ |
“c’†@—ǹ |
|
|
R005-13 |
‚ƒGƒlƒ‹ƒM[—±Žq~ƒŠž‚Ý‚Ì‘å‹C‰e‹¿—‰ð‚Ì‚½‚߂̺˜aŠî’n‚É‚¨‚¯‚鑽‹Püƒ~ƒŠ”g“¯ŽžŠÏ‘ª‚ÌŒ»ó‚Æ¡Œã‚ÌŒv‰æ |
•\Ž¦ |
# |
|
R006-01 |
Spatiotemporal variation of 3D distribution of discrete auroral arcs |
•\Ž¦ |
|
|
R006-07 |
ƒI[ƒƒ‰XƒvƒƒWƒFƒNƒgF“ì‹ÉE‹ÉŠ¥ˆæ‚Ì‘å‹C“d—£‚ÌŒ¤‹† |
•\Ž¦ |
|
|
R006-P23 |
Methods to increase the precision of the frequency of FLR in SuperDARN VLOS and the magnetospheric density |
•\Ž¦ |
|
|
R010-12 |
Atmospheric ionization impact of EMIC-wave driven energetic electron precipitation events |
•\Ž¦ |
|
|
R010-20 |
‰F’ˆüƒf[ƒ^‚ÌŒöŠJE‰ð͊‹«‚ÌüV‚ÖŒü‚¯‚½Žæ‚è‘g‚Ý |
•\Ž¦ |
|
|
R011-05 |
‘—§‹É’nŒ¤‹†Š‚É‚¨‚¯‚éƒI[ƒƒ‰ƒf[ƒ^ƒA[ƒJƒCƒu‚ÌŒ»ó‚Æ«—ˆ |
•\Ž¦ |
|
* |
R011-10 |
•ª–쉡’fŒ^ƒf[ƒ^ƒJƒ^ƒƒOAMIDER‚̉^—pŠJŽn‚ÖŒü‚¯‚½€”õó‹µ |
•\Ž¦ |
|
|
R011-11 |
GAIAƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“ƒf[ƒ^‚ÌIUGONETEDOI“o˜^‚ÉŒü‚¯‚Ä\DOI“o˜^ƒVƒXƒeƒ€‚ÌXVŒv‰æ |
•\Ž¦ |
|
|
R011-12 |
IUGONETƒvƒƒWƒFƒNƒg‚ÌŒ»ó‚Æ¡Œã‚ÌŒv‰æ |
•\Ž¦ |
|
|
R011-15 |
Œ¤‹†ƒf[ƒ^‚ð‚æ‚茩‚‚¯‚â‚·‚‚·‚邽‚߂̃ƒ^ƒf[ƒ^•ÏŠ·‚Æ‹@ŠÖƒŠƒ|ƒWƒgƒŠ‚Ö‚Ì“o˜^ |
•\Ž¦ |
’J“ˆ@M‹M |
|
|
R010-P01 |
Dawnside Surface Charging Events on the Defense Meteorological Satellite Program F16 Satellite |
•\Ž¦ |
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R011-P02 |
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’JŒ³@—Ä‘¾ |
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R004-04 |
–[‘”¼“‡“ì’[’nˆæ‚É•ª•z‚·‚éŠC¬‘w‚©‚瓾‚ç‚ꂽƒJƒGƒi‹tŽ¥‹ÉˆŸ‘Ñã•”‹«ŠE‚̌ÒnŽ¥‹C‹L˜^ |
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“c•£@x•½ |
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R005-24 |
q‹óq–@—p“d”gILS Localizer‚ð—p‚¢‚½ƒXƒ|ƒ‰ƒfƒBƒbƒN E ‘w‹óŠÔ\‘¢‚̉ðÍ |
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‹Ê‘º@—D„ |
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R006-P26 |
‚ ‚点‚ÅŠÏ‘ª‚³‚ꂽ’áŽü”gƒzƒCƒbƒXƒ‰[ƒR[ƒ‰ƒX”g“®‚̉ðÍ |
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“c‘º@T |
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R003-P03 |
Constrained inversion of MT data with seismic velocity model in the southern part of NE Japan |
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R004-01 |
Strong magnetic anomalies record the weak dynamo field of ancient Mars |
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’O@G–ç |
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R009-08 |
‰–‰»ƒiƒgƒŠƒEƒ€‚ւ̃vƒ‰ƒYƒ}ÆŽËŽÀŒ±‚Æ•¨—‰»Šwƒ‚ƒfƒŠƒ“ƒO‚É‚æ‚éƒGƒEƒƒp‚ÌŠó”–‘å‹C¶¬‚Æ•\‘w‘g¬‚̉𖾠|
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