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þüìîðÕàæàĝMagnetic fields
in the penumbracorona  áßàãÞèÞàâphotosphere:f@2014K?Kæ

B in the chromosphere: He I 1083 nm
Stokes I

Stokes Q

Stokes U

Stokes V

B = 960.5G# B = 119.2!
" B = !121.1!

Zeeman effect
B = 730.2G# B = 107.4!
" B = !158.1!
B = 578.7G# B = 103.8!
" B = !145.9!

Hanle effectB = 368.0G# B = 98.0!
" B = !147.8!
!!
!!

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"#$"
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Requirement
Goal
"#$

('. (4*1 D*0'*+ ))./ E,+ - (*/,* '=/ =@'+< 8'1; .(2/&'(21+* )*+,(A7 ./*)+A +'0*,E) 1'.()D*(,.

-./*+'0*1'.(,*D-/'1=@)ìüñċĎăďćĐĕĔ&'()*+,-./*+'0*1'.(,234ûý$""$;'+<=/*+,-./*+'0*1'.(,234Spectral profiles of He I 1083 nm

Expected pol signals in QS(Ğġ=0.12)
$#"$"#"$""#"?')/@,A1+)(819,28*=AA4$"""#"5#"

He 1083 nm ŀņÎ1ŎŵřƁŽƆůŅ­ņTYħÉÎ1ŀņİŃő
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B ~ 10 GaussŖŪƈźƆƇųƆƄrŀsķŒĻŌńĦ
ĥĥ«|ĴœŒZMÕ2 - 3x10-4. ĥvņÕ1x10-4
ĥĥĥ(0.14”x0.18”, 10-20 secŀÇŌŐœŒ=eŀ½#¦)!!

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áx­ń«|ĴœŒ«¡^ªŅ2ÂŖBgħ!!

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ĊăėċĐĉÕĒđĎăēċěăĕċđĐÕďăċĐĕćĐăĐąćÕØąđĖēĕćĔĚÕđĈÕóÝÕ÷ċĐÙþćĔĕÕďđĆćĎÕđĈÕĕĊćÕôĐĕćĉēăĎÕñċćĎĆÕÿĐċĕÕáßàãÞèÞàâoqźŚšƅŚŽƈŧŨƁŚťƈŅÂÕØāáÜàßăÙààýĖďďăēĚ!!

ýù÷ìüÜîŀ`ķōŅ
Ģ! ®dĴœĻŝŲƃŠƈŖ(,Ƈń cĴĸĿĩŒōŅŖŁŐīŒĳŁħĢ! zƂŤŲšŦƀƆĮ´ĳĽĿĩŒĺŅ3\Ņ3Ŗb­ķŒĳŁħ
!!

Measurement of B around theroots of jets provides clear
evidence of MR.

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ŐœĿįĿĩŒ
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