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3.!āÓOÁ_;!

SOLAR-CĹó!
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!

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SOLAR,Cĭ¼ƶÎĲ%ŔøƳȂƮƶĶßįġ!
EUVST (EUV Spectrograph)
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wƸƶưGĕ3(~1.4m)!

Optical Bench Unit• EUVST!

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SUVIT IFSUVIT FGPSUVIT SPPXIT (X-ray imager)

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XíāÓǷǕǥǒǗǵǼ!
Study!of!a!Fundamental!Physical!ProcessŷāÓǹǌǦǸǚ²ưƶŷőǷǕǥǒǗǵǼÏŒƱƷȆ!

YohkohHinode & SDOSOLAR-C

Spectroscopy

!彩層–コロナ高解像度
Ɣ(0.3”) ó"ǽ0&Ķß!高感度(>×10)
in spectroscopy⇒ 高時間分解能

Hara!et!al.!(2011)

Imaging
~3”

Shibata!et!al.!(1995)

Takasao!et!al.!(2012)

!内部磁気島とMHD
衝撃波構造を形成する
高速リコネクション過程を実証fŨdÓƶÏŒƱǎǥǸǑǾŊŎ!
Observations of All from photosphere to corona seamlesslyìéȄźHinodeƶÇǕǺǣ8åƶú§ĶßƷƺƱǊƲÂŢ !
ƦƞƦƪƶçŸƷ£Ɯƫ!

&ŞƱ0ĸĦƶŇ
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fŨdÓƶÏŒƱǎǥǸǑǾŊŎ!
Observations of All from photosphere to corona seamlessly• ó"ǽ0&ĶßưǃǆǅåÏŒƱāÓÏŒƶŤƷ?
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HinodeÖš0.3”,0.5”

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Chromopshere

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Hinode

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ƹƶǌǼǪǞǡ!

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Observations
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10.0

Yohkoh*1991*

SOHO*1995*

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SOHO*1995*

Chrom.,Corona,spectroscopy

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Spatial Resolution (arcsec)

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0.1

IRIS*2013*

Chrom.,TR!Spectroscopy

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Solar!UV,Visible,IR!Telescope

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spectro,polarimter!!
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100!nm!

120!nm!

140!nm!

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