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KWASAN & HIDA OBSERVATORIES

GRADUATE SCHOOL OF SCIENCE, KYOTO UNIVERSITY

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2006 ;@@° 5 ¶ 29 ·*¸ 6 ¶ 2 ·E¹ 4 ·ºM»7¼7i7½c¾K®[¿7ÀP³M°g¦Ác'7·ºK®[Â 500 ÃÄ 7JK®[ÅIÆ@Ç9ÈÉcdÊ#ËQQÌ¹YÍ7Î@®[Ï7ÐP³M¨`6\Í7ÎP³M¨YËQQÌe[Ñ7Ò,¹KÓÔOÊÕG°9fÖ1Õ@¹KËgcÌ,3E×I©GØG°`ÙÚqÛ`Õ#/62006 05 30

Time OBJECT PA Inc radius WL(nm)

07:55 QR 9 99 3.00->4.30 538.0(CI), 457.1(MgI)

16

2006 05 31

Time OBJECT PA Inc radius WL(A)

00:29 NOAA0889 109 19 5.00->6.30 538.0(CI), 457.1(MgI)

01:26 QR 538.0(CI), 457.1(MgI)

01:32 LR 19 19 14.53 538.0(CI), 457.1(MgI)

01:57 NOAA0887 538.0(CI), 457.1(MgI)

04:49 NOAA0889 112 22 4.40->6.10 538.0(CI), 457.1(MgI)

05:09 SGB 180 90 4.00->5.30 538.0(CI), 457.1(MgI)

05:27 NOAA0887 139 50 2.20->3.50 538.0(CI), 457.1(MgI)

05:46 DFbarb 318 107 13.28 538.0(CI), 457.1(MgI)

05:55 DFbarb 317 131 13.38 538.0(CI), 457.1(MgI)

06:20 344 344 0.06->15.04 538.0(CI)

07:00 NOAA0889 112 22 4.40->6.10 538.0(CI), 457.1(MgI)

07:44 QR 0.10->1.40 538.0(CI), 457.1(MgI),

10830(HeI)

2006 06 01

Time OBJECT PA Inc radius WL(A)

00:29 DF 320 49 12.00->13.30 538.0(CI), 457.1(MgI)

01:06 DF 313 43 13.30->15.00 538.0(CI), 457.1(MgI)

QR: Quiet Region

LR: Limb Region

SGB: Super Glanule Boundary

DF: Dark Filament

barb: foot point pf the dark filament

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Reference: Imada, A., c Nogami, D. d1e 8 f; <Åg , 2006, PASJ, 58, L23

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Reference: Aungwerojwit, A., - Nogami, D. ./ 15 01*2 , 2006, A&A, 455, 659

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Reference: Isobe, Miyagoshi, Shibata & Yokoyama, 2006, PASJ, 58, 423

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24

"!#$%&('*)+,.-./ +F%K1032.4657.8:9.;1<>=@?V?XA<CBEDAF@G2k>9&.H()JAJIK6$/9lML0ENO.P ^gnp?q[+, RQ.S.T,AVU[k[9JW.XMY[Za.E\.].^`_badcA_be.f!kbg>h[ZMi@j[k.l>F:Wnmo Z.prqAs@tnuRadc*vxwnuRadcCFzyU[\.].^`_b|.AqVUru~rcrAc6W`ms.n_C FZ6 N O. Aqr.SM:c oE e.>Fb[[email protected]. ¡Y¢s@|._R£.¤¥v.v¦hq`[ P§ ...g¨.©j oEª.« Fz¬MY[ZJr®c¯As°|..±.²Vq o vacVZR\.].^n_R³.4gM¡´¶µ.·Aq o v¸qr¹ºnY®~u o AiEqAszN O. _b\.]..»A¯r..n_R¼.½A¾r.S¡:c o [.¿n_RÀÁÂv¸¯JÃÁ`Ä¢_A®>F@¬MY®ZJ[[.¿`_btMz¯Jadcg.tuJ\]^`ÅÆ¢tÈÇÉsR_J¼½V¯6aVc.g.wub\d]^V¾6ÊË`¾AÌÂÍ¢Z6Î°6ÏÐ¢Ñ _R\..Ò.ÓA¾.¯As°Ô.Õ.I.Ö`_b×.¿..».g`._b.ØAqrÙ.ÚVVÛ[ÜÂF:yU`v[FÝ iEÞ.qÂY¢Zr¢adcgwnuR.fA¯[email protected][ZrßAàVD<.áâ`ãr ª.ä F@¬j[å.ÀnszadcgtnuR.fA¯r\.æ.çgM¡´¶èùbé.êAqrëìnY[s[<Jí6îïAð`v°uñ6c o`òó.ô _b\.6Ò.ÓÂF@Y[Z6,dõö ¾¯VsA¢c*iz_ ½>F÷ùø®ú filament channel, flux rope, sigmoid v:u1ÍZJûü ¾6ýþ@c o°ÿ _ºJqÙu.~¡Y¦Z6

a) b)

c) d)

: 9.; Vq1¡´¶i¸cVZR\...Ø v j o ÏAÐ®Ñ \.n_Rý.þAA¯radcgtùbf`¾VsV¯6aAc.gwubfMF¬j

Reference: Magara 2006, ApJ, 653, 1499 ( )

25

!# ¾ .¡:c o â « ç _..ÒÂFz Ý j o v¸¯ !" q$#&% o' ()n_ +* ¾dÌ o r®cMø@¾d_&,-A¾.¯/.01.g2>h43.æA&5 67 ¾AÌÈ´ sRûü89:Aq$#6u6~Ch[s<;= .01?>@89/ACB?DFEHGJIzÆ[q?K¡Íz~ â « gý.þ¡:cd~u o Vh.Ídv¦h¦sïLNMO5 NP ! A¯r£@Q¾du o h PP × «q * u6~¯/R. S PUT gVnuJ`Û[Üj oW YXZ\[] @âng^¡ÇÉsø`_s®tnuUa.ç.b g\c\dj o vEÞùizs !õ >$e\fgDihkjmlJ$DEnMbq> o ,\-dg\oqp¦u6Þ*i°¾AÌ o ¢¾dsrefstA¾.¯ u.æ PUvw Þ¡[email protected]\z| ôNP â [<~ I â4 ¾1Ä¢~uu¡v°u¥sAq/kp¢s 1991 Vq<E$_ Geotail =\.qpk_U PU |<nAÞ$$ Vú\_/4 7 ã&r×\CÆ PFF¡ <¢£NP J¤O|¥Oy%/5¦q§ i¨4©Crª«4_U¬® PU¯° ©`±²qpk³k´µ P&¶· n¸N_/¹4º?³`»5 ¦ P¼½|¾ |¿c b nÀNÁ¨`_Â\³Ã.01ÄÅÆm$#&%¨`ÇÈOÉgÊË [/~ IÌÉ P&Í?ÎÏÐ Ñ «4_/FÒ/ÓkÔ/Õ ×Ö ³&Ø©@z|nÙ P ÇÈOÉgÊË [/~ IÌÉCnÚipOÛ@ªF¨ÜgÝßÞ PÓJz$Mià$á?ª?Û@³/âãHäåàæçèé êëæçèìíîïàðñòUóô\õ éöø÷4/ù|¨Ã¿?úûü4À$Áý êÿþ ³|÷ë<âgãäåõ?g¤kª|¥U³O©@á/³ æçèéõ?¤kª¥ å ê å F (E) ∝ E−Γ ¨ Γ ÷rõ § ª³< »\õ ¦ Û\ªF¨/ õ m©¨4@þ?³ Nª!ím#"Óã%$ ½ Ëè\õðñ$&'() *,+ ü-/. 0"|Óøã$ ½ Ë1 + âãHäåü2 Û\ªF¨4"|Óã3$ ½ Ëè\õðñ$&'54F¤@¨361 +78 ê!íò:9;³=<âãHäå³=<æçèéø÷ 4 åò>.4á¤ ?A@i¤ Ö ê G=5.0-3.5 ÷ ³B1+C7#8 4C?CADECF|òGIH0JCK Û@ªg¨ (G=3.5-3.0) LU´@ðò ¶\· ü MCNOP0>³QCR|òSUTAVW ã:XŃNò&æçè4@ò&»Y ¦ Ï Ø/òZõm©\[ õ?¸].3Pi¨%L|ý^3_:>|³,àIb#cd HAe\fæçè ê þgh9ø÷i4?Nâgã äå?A<Nªò04m³ ¦ õjªkò/^mln § Pi¨ õN³A1+ üBI_Û\ªPA>oò * [p4? ªLm¹Oý³qrs,tsæçè4/»Y\õ ¦q§ Piü^xõÕIv\ª:wyx?Az. Ö| Ø4-«4ý&õN³~qrs,tsóôò:Av&îï<©y. æçèé\õ0 §Ö ³Co\ò@ý\Â ¦CC õj Ö v«OÛ@ªg¨(C)\û@õ/Û¤Jý ê þpF÷L

ck

Super IPS

loop-topenvironment

MA

θB

n [dg

r]

Spectral Index Γ

þ : å|ò Í\Î\Ï\Ð ^

Reference: Oka, M. et al., Whistler critical Mach number and electron acceleration at

the bow shock: Geotail observation, 2006, Geophys. Res. Lett., 33, L24104.

( C )

26

! "#$%

à,@'&4@ò)('*'+', - b#c d). 4?m³,@'&?òUóôü0/^ Û 1030erg kò21@5vÇ@ÈÉqÊ@Ë&õ Ï4365 P67u ^Ãõ98g.PNÛ;:<7 Lo@òmÇ@ÈÉqÊ@Ë Ï=3 ¾?>'@ ÔBA0?DC/ó=Eíò\áv9FHGC_ - ó'&JI?KJÈ X VWML . H!N'70kò^%O7PO\õDC?Q'Rò:àTS'U'VrH<N7PS'UTW'X4Gy.ZY'EH#v[rÛ9:\7L G v/õ .0Coò2]'^HmáH:Û?`_ 5 P$ý)a/kcb:ALdIeK)fX VWcL!g >h@ji AH$áh:Û?4C&ó'EíNò@áv9F2k 7Pl 4@ò Joule m'nHN'7po'f?qsrjtTu 3 üev]Ô7 Sweet(1958) ^ Parker(1957) ò'w)x2q4yCIeKzf X VWPLHN [|=~ 5 P74æ@çmèIHN47To=fTqr9t2u 3 õ ^ O\7 Petschek(1964) ò4w`xHq v õI-\7 õDC ò'w)x`qNõàIb#c d üeO4\47nòHGH@áH:H@ò)SjU4G.rò20FW'X?s0#v9:ALo u4h''4?4Cpo'fpq<rjtTu 3 ò)4Gy.ZS'UAv2 * ü0I_!7Au^ü ý0L` azS9U9VCrN fufxò2 X í9=95HsN97MxtC'&9,9VCr GOES 4HI_y.3PNý`

aòh X í4@öò`x\tC0à)S4U=V#r SOHO Hj4 5 Pý MDI HN=7%R=mó@ôòxt?ü?B:'4C 2000 R RC |ò` a b5c d 77 |òz6 i CH¡Cs#$'¢'t?q<Cnó\ô|ò@5 ^0:<[kýh£#w=¤qüpUF oP].`ò52¥qüp¦§@ý/ðI4BCb5c d 4$ò4o=fTqr=t)u 3 üpÖ)¤C©IK`f/X V W?L cztª ò`«4¬=u4iüp®[OýLo@òh¯=°CIK`f/X V WeL c)tªÃòGJ±³²5? Petschek w2xhq<´2µ=UCG^?¶z·=¸B´`S9UCG=¹9ºd»3PD¼`¹C5o9´K4½T¾=´`£w4¤ (¿=& Reynolds À ) H'ÁO\70Â=Ã=ÄBÅ Petschek w`xHqÆ0´hµ4U©ÆcÅjÇÈÉCBÊË4ÌSweet-Parker w2xhq<´\N<ÍÎÈh:2Â9Ã=ÄsÏ?ÐÑBÒÆzÏ?ÓÔËT¼HÕ

Ö × I?K2f<ØhÙsÚ LÛ t6ª MA ´`¿9Ü Reynolds À Rm Ý ÁÑÞMÂ=Ã9ÄsÏ?ÐËT¼ß)´HÕ`à;á4âÅ'x!t\)´!ãäZåPæä L9ç;è â MA ∝ R−0.8

m C24âÅ Petschek wHxjq Ý N4Þeé4êë µ=UÏp¨Ñ è â MA ≤ π/ [8 ln (8Rm)] ì;ísÞ?Õ`î4âDÅ Sweet-Parker whxHq\ìD´hÂ=Ã4ÄMA ∝ R−0.5

mÏe¨ÑT¹Bï Sweet-Parker w)x`qì`µ'UðcñÞò?ózf<Ø2Ù\Úcô Û tªõ´)ö4ÅÒ

´ è â÷Éõß 5 ø;ù ú ðpûHÕ

Reference: Kaori Nagashima & Takaaki Yokoyama, 2006 ApJ, 647, 654-661

(üýþ ÿ )

27

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28

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29

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30

Coronal Heating by Nanoflares and Alfven Waves, PredictingObservational Features (Master Thesis)

Alfven waves are good candidates to heat and maintain the solar corona to the observed

few million degrees (Alfven 1947, Hollweg 1982). Another appealing candidate is the

nanoflare heating, in which energy is released through many small reconnection events

(Parker 1988; Priest et al. 2002). Distinguishing the observational features of each is

an extremely difficult task. In this thesis we address this problem by setting up two

coronal loop models using the CIP-MOCCT scheme (Evans & Hawley 1988, Yabe &

Aoki 1991), each one heated by one of the two mechanisms. The first model is a 1-

D HD code in which numerous heating events are input randomly (uniformly) along

the loop (nanoflares). The second model is a 1.5-D MHD code in which, in addition

to nanoflares, Alfven waves are also created, following Moriyasu et al. 2004, by sub-

photospheric motions at both footpoints. The waves convert non-linearly to slow and fast

modes that dissipate their energy through shocks. Both models reach a uniform state that

satisfies the RTV scaling law. Alfven waves are found to produce a more dynamical corona

with strong slow and fast shocks. The transition region is pushed upward by magnetic

pressure from the waves reaching heights of 10 Mm. On the other hand the uniformly

distributed nanoflares have a smoothening effect permeating the corona with weak acoustic

shocks. The heating events increase locally the temperature but thermal conduction is

high enough to distribute efficiently the heating throughout the loop. The transition

region is less dynamic and oscillates with periods close to the observed chromospheric 3

minute oscillation. We construct for both models the intensity flux distribution as would

be observed with Hinode/XRT. The Alfven wave intensity profile is more spiky due to

the stronger shocks. Hence, the general picture of nanoflares, being ubiquitous, sporadic

releases of energy is here closer to the Alfven wave model than the own ”Nanoflare” model.

However, footpoint concentrated nanoflares can create more dynamic coronas (Taroyan

et al 2006) and have a better observational support (Aschwanden 2001) but are left as

future work.

j : Density profiles along the loop and Intensity fluxes at the apex of the loop for Nanoflare

models with (left two figures) and without (right two figures) Alfven waves.

(Antolin Patrickp

)

31

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32

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¢y_ò _hgikj[j Bl! UVm d8n ¹ o Z 6p ²T³ !

q - :ÐDßsÛH x_ (r8s )

ªÜ«t TRACE

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( 0 Ä î~ w & ) t% ¹7ï º £¢ _ « ° N 7Ë F Ó° ÐÜß]Û.H x& ')? o Ê|$Tî (∗

;8 î) £¢* pB ÿ £ !

Reference:

1. Kaori Nagashima & Takaaki Yokoyama, 2006 ApJ, 647, 654-661

2. Kaori Nagashima et al., 2007 ApJ, 668, 533-545

("| )

33

Æ7Ç Ð>Ñ@Ò ÄDÍ¥M o Oï"! =$# ~ 3&% t #(' F$)l°+* 6 t(,.- M o Dï0/ ! C$1 ° (243 î ú65 · !7)$89 "! ;: - M o Dï0/ <=?> : ' =?> ò@ ,BA 5kj Bl! DC !FFE$G ! : Z *(H (IJ6KLM'N ï Ý 'MO !

2004 ¾ 11 ¿ 10 â 11:00JST P *(QFR(S L ù Hα T ïVUMW0XBY(Z6[6\ ' GOES ]6^X2.5 _.` Y Zba @dcDeDfhgjik(lD! -4mDn+-Do;nqpDrDs 'tBu G;v :;w , 1Dx 9qyz T4U$W|XY+ZD[B\6~6*D ';+tBu ,h. a v a ZD[B\Bz+ik(lq~6 =W+!| 1 9&*&h , ~ w $ E v a(¡6¢ £ Hα

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-

Peak intensity of flare kernel

2004/11/10 Ha (Sartorius) TRACE(1600A),contour:RHESSI(25-100keV)

particle precipitation

«7<>=Hα w C IV

£ Ã$Ä$Å § Ó?" Mi6k.l À «A@B= ¤ B¥|¦DC ä _?E p$÷

Reference:

Shibata,K. and Tanuma,S.,2001,Earth Planets and Space,53,473

Benz,A.O. and Aschwanden,M.L.,1992,in Proc. Eruptive Solar Flares, IAU colloq.No.133,106

Karlicky,M. et al.,2000,Solar phys,195,165

Kliem,B., Karlichy,M. and Benz,A.O.,2000,AA,360,715

(F8G H8I J )

34

! #"$&% '() *+

Height Dependence of the Gas Flows in an Ellerman Bomb

2004 , 11 - 24 ° $ y À/.103214 NOAA10705

665 37 & ¹ °4ì986 p ê t6u Ø;:3<1=1>6? Ý9@ g ² yDz"A5 17 ¹ ê1B3C ä Û Ø;D E Bp ê °º GFEFv òjw ¨ Ý6H y.z TiIIJI9K$Å w Hα

¡ Å ØML 8D À ê9B wON C ä Û Ø F E$yJPQ À êRB Ý ~ 0.2 km s−1/SUT ÀVN Ý ~ 1-3 km s−1

/WYX Ø tDu Í yz ò /P Q ºÁÀ Z5 [7 0 ¹ 6 ¥+¦ ® r¯ ~RS6 ê[B Ý ú ò ²ü18 v wO\1]MÝH v (

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5 97 + ¹ `_9a4 C ä $Ø ð4ñ v òjw ~ À 5 97 + ¹ `b9ced à Ýhá vf a " $(¥#g&>( Øih[j vkS Ý ml[n Ýhá v7z

MHD Modeling for the Global Solar Corona

; $9o;p /_UqUr MHDDØ ðhñ sMt E ° À CIP-MOCCT u ØVL 8Ut À 3 vUw MHD

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(ë ì[í î )

35

5.5 a. ³[´ b. ³[´ c.

(1) Ú ³[´ (17GS0208)

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(2) 2* µ !3 ¶ ³[á. 3m 456789 Ê:;< >='? µA@CBDFE Û À[Á ³[´b. #%$'& Ú ( 2* : GIHKJLNMPOFQSR ³[´T )

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36

6 6.1 1.+ I :

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Â+$rÃDNumerical and Observational Studies of Coronal Mass Ejections and Associated

Phenomena E( ¡ G!¯°±+²GFIHKJ ÏML ij!¿À+Á'ac%Á ª« )

Ibrahim A. A.DLong Term Simulations of Astrophysical Jets; Energy Structure and Quasi-Periodic

Ejection ENPO RQTSPMP6UKV*>G0XW+Y'>[Z]\ ; ^_K_[`'a1Fcbde+Áf%²g

• o2@A (h5 18 i 9 jBC )

Antolin P.DCoronal Heating by Nanoflares and Alfven Waves, Predicting Obser-

vational Features E• k2@A (h5 19 i 3 jBC )lnm o9p Drqns Á nt[uwvTxnyznn|IÄ Y~T0]WYX/MZ\n L

X K[MEUM D ^_X[`n'+M /¡T¢n£ L¤M¥¦ Y$§M¨©ªE«¬ ® D°¯ \]±²~³ ¤M¥¦ Y$ ¦ 8/n´cT a1FIµ t¶· E¸¹ º» D ¤K¥¼½ ¡<~¾ L ¿ FwÀ98-:<;6ÁÂÃÄEÅMp¬ Æ DÈÇ VÉ<¡/~¾ L ³RY--Ê9 MHD ËÌK¡ L σ ÍÎÏÀ9ÐÑE

37

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8. D ^Î©ª S. 35D S2 (¤M¥

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ST UVW(=d : > 2 & )

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38

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39

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(DST,SMART), TU ³C´¶µ V , Mees

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(DST), Hinode(EIS), SoHO(CDS)

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the corona in XBPs”

41

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798 • 4 Q 10

ûB.V. Jackson (Center for Astrophysics and Space Sciences, University of California,

San Diego: USA)

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H. Park (Princeton Plasma Phys Lab, USA)

• 11 Q 8û

K. Hayashi (Stanford Univ, USA)

• 11 Q 20û

S. Yashiro (Catholic Univ of America & NASA Goddard, USA)

• 12 Q 4û

D. Summers (Univ of Newfoundland, Canada)

• 12 Q 6û

M. Agueros (Univ Washington, USA)

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Y. Mizuno (NASA Marshal, USA)

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M. Linton (Naval Research Laboratory USA)

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Magnetospheric Substorms as a Basis of Space Weather Research P2v#w

8.5 X~96 1. O - z V K 3 LV \ W

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2._4` OP ' h4 2007

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43

LOC,SOC,

1. IAU Symposium No.233 ”Solar Activity and its Magnetic Origin”

2006 D 3 ? 31 s –4 ? 4 s (Cairo, Egypt)

SOC, Session-chair (xk yz )

2.en f O 3 \

2006 ! 5 ? 14 s –15 s ("#%$&' )() ! $*+ (xk yz )

3. AOGS 2006 ST11–ST14 ”Onset of solar flares and coronal mass ejections”

2006 ! 7 ? 10 s –14 s (Suntec, Singapore)

co-convener(xk yz )

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4.1 E2.3/D2.6/E3.6 ”Energetic Particles and Magnetic Reconnection on the Sun

and in the Heliosphere” dupity organizer, session-chair ( xk yz )

4. 2 D2.2/E3.2 ”Magnetic Coupling in Solar and Stellar Atmospheres”

organizing committee ( xkryz )

4.3 PSW1 ”Space Weather: Observations and Modeling for Applications and

Operations” organizing committee ( xk yz )

5. IAU General Assembly, JD01 ”Particle Acceleration – From Solar System to AGN”

2006 ! 8 ? 14 s –25 s (Prague, Czech Republic)

organizing committee ( xk yz )

6. 2nd East Asia Numerical Astrophysics symposium

2006 ! 10 ? 31 s –11 ? 2 s Taejeon (Korea)

SOC, Session-chair (xk yz )

7. CAWSES International Workshop on Space Weather Modeling (CSWM)

2006 ! 11 ? 14 s –17 s The Earth Simulator Center (Yokohama, Japan)

co-chair, session-chair (x9k yz )

8. SUPERNOVAE CONFERENCE 2007

-, . )/ ' E4G 01 A3254 op67 2007 ! 2 ? 1 8 –3 8 (9 )57 () ! $ ;: < (=?>A@B )

9. The CAWSES workshop on Comparative Study of Solar Flares and Magnetospheric

Substorms as a Basis of Space Weather Research

2007 ! 3 ? 18 8 –20 8 Fairbanks Princess Riverside Lodge (Fairbanks, Alaska)

co-chair (=>A@B )

44

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=> @B

45

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11.1 ÄQÅ2006 ÆÇdÈbÉ4ÊJGËÌ¿ÍdÎÏÐÑ (1) Aungwerojwit, A.56, Gaensicke, B. T.56, Rodriguez-Gil, P.56, Hagen, H.-J.35, Araujo-

Betancor, S.40, Baernbantner, O.43, Engels, D.35, Fried, R. E.33, Harlaftis, E. T.47, Mislis,D.55, Nogami, D.1, Schmeer, P.32, Schwarz, R.53, Staude, A.53, Torres, M. A. P.36

Dwarf novae in the Hamburg quasar survey: rarer than expected, 2006, A&A, 455, 659

(2) Imada, A.14, Kato, T.14, Monard, B.34, Retter, A.51, Liu, A.50, Nogami, D.1

The 2005 July Superoutburst of the Dwarf Nova 2QZ J021927.9-304545: the SU UMaNature Confirmed, 2006, PASJ, 58, 383

(3) Imada, A.14, Kubota, K.14, Kato, T.14, Nogami, D.1, Maehara, H.32, Nakajima, K.32,Uemura, M.25, Ishioka, R.18

Discovery of a New Dwarf Nova, TSS J022216.4+412259.9: WZ Sge-Type Dwarf NovaBreaking the Shortest Superhump Period Record, 2006, PASJ, 58, L23

(4) Isobe, H.23, Miyagoshi, T.3, Shibata, K.1, and Yokoyama, T.23

Three-Dimensional Simulation of Solar Emerging Flux Using the Earth Simulator I. Mag-netic Rayleigh-Taylor Instability at the Top of the Emerging Flux as the Origin of Fila-mentary Structure, 2006, PASJ, 58, 423.

(5) Koide, S.17, Kudoh, T.18, Shibata, K.1

Jet Formation driven by Expansion of Magnetic Bridges between Ergosphere and Diskaround Rapidly Rotating Black Holes, 2006 Phys. Rev., 74, 44005.

59

(6) Kozu, H.1, Kitai, R.1, Brooks, D.H.48, Kurokawa, H.1, Yoshimura, K.42, and Berger, T.E.41

Horizontal and Vertical Flow Structure in Emerging Flux Regions, 2006, PSAJ, 58, 407

(7) Magara, T.1

Dynamic and Topological Features of Photospheric and Coronal Activities Produced byFlux Emergence in the Sun, 2006 ApJ, 653, 1499.

(8) Masada, Y.1, Sano, T.5, Shibata, K.1

The Effect of Neutrino Radiation on Magnetorotational Instability in Proto-Neutron Stars,2007 ApJ, 655, 447

(9) Masada, Y.1, Kawanaka, N.12, Sano, T.5, Shibata, K.1

Dead Zone Formation and Nonsteady Hyperaccretion in Collapsar Disks: A Possible Ori-gin of Short-Term Variability in the Prompt Emission of Gamma-Ray Bursts, 2007 ApJ,663, 437

(10) Miura, N.9, Kobayashi, T.9, Sakuma, R.9, Kuwamura, S.9, Baba, N.27, Hanaoka, Y.18,UeNo, S.1, Kitai, R.1

Solar Adaptive Optics System Based on Software Control, 2006, Optical Revies, 13, 338

(11) Nagashima, K.1, and Yokoyama, T.23

Statistical Study of the Reconnection Rate in Solar Flares Observed with Yohkoh SXT,2006, ApJ, 647, 654.

(12) Oizumi, S.8, Omodaka, T.8, Yamamoto, H.8, Tanada, S.8, Yasuda, T.8, ARAO, Y.8,Kodama, K.8, Suzuki, M.8, Matsuo, T.8, Maehara, H.32, Nakajima, K.32, Dubovsky,P.A.39, Kato, T.14, Imada, A.14, Kubota, A.14, Sugiyasu, K.14, Morikawa, K.32, Torii,K.5, Uemura, M.25, Ishioka, R.18, Tanabe, K.6, Nogami, D.1

Long-term monitoring of the short period SU UMa-type dwarf nova, V844 Herculis, 2007,PASJ, 59, 643

(13) Oka, M.1, T. Terasawa23, Y. Seki3, M. Fujimoto3, Y. Kasaba3, H. Kojima13, I. Shinohara3,H. Matsui49, H. Matsumoto13, Y. Saito3, and T. Mukai3,

Whistler critical Mach number and electron acceleration at the bow shock: Geotail obser-vation, 2006, Geophys. Res. Lett., 33, L24104, doi:10.1029/2006GL028156.

(14) Sudo, Y.27, Baba, N.27, Miura, N.9, UeNo, S.1, and Kitai, R.1

Application of self-deconvolution method to shift-and-add solar imaging, 2006, AppliedOptics, 45, 2707.

(15) Tanuma, S.1, Shibata, K.1

Oblique Shocks in the Magnetic Reconnection Jet in Solar Flares, 2007, PASJ, 59, L1

2006 ÆÇdÈbÉ4ÊJGËÌ¿ÍdÎjÑ (1) Asai, A.19, Yokoyama, T.23, Shimojo, M.19, Masuda, S.24, Shibata, K.1

Initiation of CMEs by Magnetic Flux Emergence, 2006, Journal of Astrophysics and As-tronomy, vol. 27, no.2 & 3 P. 167–173

60

(2) Chen, P.F.44, Fan, C.44, Shibata, K.1

Why are there stationary EIT wave fronts, 2006 Advances in Space Research, Volume 38,Issue 3, p. 456–460.

(3) Terasawa, T.23, M. Oka1, K. Nakata23, K. Keika15, M. Nose16, R. W. McEntire38, Y.Saito3, T. Mukai3,

’Cosmic-ray-mediated’ interplanetary shocks in 1994 and 2003, 2006, Advances in SpaceResearch, 37 (8), 1408-1412.

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(23) Nishida, K.1, Shimizu, M.1, Shiota, D.1, Takasaki, H.1, and Shibata, K.1

MHD Simulation of Plasmoid-Induced-Reconnection in Solar Flares (oral)

62

(24) Nagashima, K.1, and Yokoyama, T.23

Statistical analysis of the reconnection rate in solar flares (oral)

(25) Shiota, D.1, Isobe, H.23, Chen, P.F.44, Yamamoto, T.T.18, Sakajiri, T.31, and Shibata,K.1

Self-Consistent MHD Modeling of a Coronal Mass Ejection, Coronal Dimming, and aGiant Cusp-Shaped Arcade Formation

36th COSPAR Scientific Assembly ( h ) 7 j 16 k –23 k(26) Kurokawa, H.1, Ishii, T.T.1, Ueno, S.1, Nagata, S.1, Kitai, R.1, Shibata, K.1

Close causal relation between emergence of twisted flux rope and strong flares (oral)

(27) Shiota, D.1, Isobe, H.23, Chen, P.F.44, Yamamoto, T.T.18, Sakajiri, T.31, and Shibata,K.1

Self-Consistent MHD Modeling of a Coronal Mass Ejection, Coronal Dimming, and aGiant Cusp-Shaped Arcade Formation

(28) Asai, A.19, Ishii, T.T1, and Gopalswamy, N.45

Anemone structure of AR NOAA 10798 and related geo-effective flares and CMEs

(29) Kawamichi, T.1, and Shibata, K.1

A simulation on protostar flare and the expected hard X-ray spectrum (oral)

(30) Shibata, K.1, and Kurokawa, H.1

CAWSES Related Projects in Japan : Grant-in-Aid for Creative Scientific Research ”BasicStudy of Space Weather Prediction” and CHAIN (Continuous H Alpha Imaging Network)(oral)

(31) Yamauchi, Y.1, Wang, H.37, Moore, R.L.46

H-alpha and UV chromospheric jets from BBSO/TRACE observations (poster)

3rd CAWSES Science Planning Meeting ( h ) 7 j 23 k(32) Shibata, K.1

CAWSES theme2 space weather : science and application – report of recent activities –(oral)

Western Pacific Geophysics Meeting ( h ) 7 j 24 k –25 k(33) Shibata, K.1

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(35) Asai, A.19, Ishii, T.T1, and Gopalswamy, N.45

Anemone structure of Active Region NOAA 10798 and related geo-effective flares/ CMEs(oral)

(36) Hagino, M.1, Kitai, R.1, Shibata, K.1

SMART Observation of Magnetic Helicity in Solar Filaments (poster)

(37) Ishii, T.T.1, Nagashima, K.1, Kurokawa, H.1, Kitai, R.1, Ueno, S.1, Nagata, S.1, Shibata,K.1

Magnetic Field Configuration and Evolution of a Highly Flare-producitve Region NOAA10808 (2005-Sep) (poster)

IAU Symp238: BLACK HOLES: FROM STARS TO GALAXIES –ACROSS THE RANGE OF MASSES

(38) Uemura, M.25, Kato, T.14, Nogami, D.1, Imada, A.14, Ishioka, R.19

Peculiar Outbursts of a Black Hole X-Ray Transient, V4641 Sgr (poster)

IAU Symp240: BINARY STARS AS CRITICAL TOOLS AND TESTS INCONTEMPORARY ASTROPHYSICS

(39) Imada, A.14, Kubota, K.14, Kato, T.14, Nogami, D.1, Maehara, H.32, Nakajima, K.32,Uemura, M.25, Ishioka, R.19

Discovery of a new dwarf nova, TSS J022216.4+412259.9: WZ Sge-type dwarf novaebreaking the shortest superhump period record (poster)

(40) Nogami, D.1, and Mineshige, S.12

Frontiers of transient phenomena in X-ray binaries and cataclysmic variables investigatedby a high-speed CCD camera and an automated monitor telescope (poster)

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MHD Simulations of Flares and Jets in the Sun, Stars, and Accretion Disks (invited talk)

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Particle Acceleration by Shocks and the Whistler Critical Mach Number (oral)

(89) Nagashima, K.1, Ishii, T.T.1, Okamoto, T.J.1, Yokoyama, T.23, Shibata, K.1

The trigger mechanism of flares occurred in the most flare-productive active region duringSolar Cycle 23 (poster)

(90) Nishitsuka, N.1, Nishida, K.1, Shibata, K.1

The test of the Fermi acceleration of the plasmoids passing through the fast shock (poster)

(91) Nishida, K.1, Shimizu, M.1, Shiota, D.1, Tasakaki, H.1, Shibata, K.1

An MHD Model for Impulsive Flares Focused on a Correlation between Plasmoid Speedand Reconnection Rate (poster)

(92) Magara, T.1

Photospheric and coronal activities dynamically produced by flux emergence (oral)

(93) Otsuji, K.1 and Kitai, R.1

The measurement of ascent speed of the ephemeral active regions using the cloud model(poster)

(94) Shiota, D.1, Kusano, K.21, Miyoshi, T.25, Nishikawa, N.21, Shibata, K.1

Three dimensional MHD modeling of Coronal Mass Ejections (oral)

(95) Ueno, S.1, Hagino, M.1, Dun, J.P.1, Otsuji, K.1, Nagata, S.1, Nagashima, K.1, Ishii,T.T.1, Kitai, R.1, Shibata, K.1, Kusano, K.21

Investigation of the Spatial Correlation between Solar Flare Kernels and PhotosphericMagnetic Field Configurations by using the SMART at Hida Obs. (poster)

(96) Kurokawa, H.1, Ishii, T.T.1

Observational Evidences of Emerging Twisted Magnetic Flux Ropes in Strong Flare Re-gions (oral)

(97) Yamauchi, Y.1, Magara, T.1, Marubashi, K.20, Oka, M.1, Otsuji, K.1, Nagashima, K.1,and Shibata, K.1

Comparison between Characteristics of Filament Eruptions and Magnetic Flux Ropes(poster)

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Science (Bangalore, India) 11 Q 27 R –12 Q 1 R(100) Ueno, S.1, Shibata, K.1, Kitai, R.1, Nagata, S.1, Kimura, G.1, Nakatani, Y.1

Chain-Project and Installation of Flare Monitoring Telescopes in Developing Countries(invited talk)

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Matsumoto13, Y. Saito3, and T. Mukai3

Shock Acceleration of Electrons: GEOTAIL Observation

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Solar Activity Affecting Space Weather and CHAIN project (invited)

International Conference on ”Challenges for Solar Cycle 24”(PRL, Ahmedabad, India) 1 22 –25

(110) Isobe, H.23, and Shibata, K.1

Reconnection in Solar Flares: Outstanding Questions (invited)

69

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Solar Activity Affecting Space Weather and CHAIN project (invited)

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Magnetohydrodynamic Jets from Stars and Disks (invited)

Polar X-ray Jets workshop ( ) 2 3 (114) Shibata, K.1

Magnetic Reconnection Mechanism of X-ray Jets (invited)

JSPS FEGIH 68J (/EKL , M F ) 2 7 –10 (115) M.Hagino1, Y.Hanaoka18, T.Sakurai18, S.Ueno1, D.Suzuki30, R.Kitai1, K.Shibata1

Magnetic Field Observation: SMART vs. SFT/MTK vs. SST/KSW (oral)

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Spicule formation from torsional Alfven waves and Nanoflares: Comparison with observa-tions

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(130) Shibata, K.1

MHD Shock Waves in the Corona (invited)

(131) Oka, M.1

GEOTAIL Observation: Shock Acceleration of Electrons

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(132) Magara, T.1 and Shibata, K.1

MHD Simulations of Plasma Ejections in the Solar Atmosphere (invited)

(133) Nishitsuka, N.1, Nishida, K.1, Shibata, K.1

Fermi acceleration of the plasmoids passing through the fast shock (poster)

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71

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(137) Ueno, S.1, Shibata, K.1, Ishituska, J.K.52, Ishituka, M.52, Kimura, G.1, Nakatani, Y.1,Kitai, R.1, Nagata, S.1, Otsuji, K.1

CHAIN-Project and Installation of the Flare Monitoring Telescope in Peru

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(138) Shibata, K.1

Introduction to Solar Flares: Questions from Solar Physicist (oral)

(139) Oka, M.1

Particle Acceleration by Shocks (oral)

(140) Okamoto, T.J.1, and SOT team

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11.3 ^`_`a`bdc`eCONTRIBUTIONS FROM THE KWASAN AND HIDA OBSERVATORIES2006 fhgjilknmpo2q=r Î (ë"Î ìs"æt g5u ª )

No. 503 Aungwerojwit, A., Gaensicke, B. T., Rodriguez-Gil, P., Hagen, H.-J., Araujo-Betancor, S., Baernbantner, O., Engels, D., Fried, R. E., Harlaftis, E. T., Mislis, D.,Nogami, D., Schmeer, P., Schwarz, R., Staude, A., Torres, M. A. P.

Dwarf novae in the Hamburg quasar survey: rarer than expected, 2006, A&A, 455, 659

75

No. 504 Imada, A, Kato, T., Kubota, K., Uemura, M., Ishioka, R., Kiyota, S., Kinugasa,K., Maehara, H., Nakajima, K., Monard, B., Starkey, D. R., Oksanen, A., Nogami, D.

The 2003/2004 Superoutburst of SDSS J013701.06-091234.9, 2006, PASJ, 58, 1431

No. 505 Imada, A., Kato, T., Monard, B., Retter, A., Liu, A., Nogami, D.

The 2005 July Superoutburst of the Dwarf Nova 2QZ J021927.9-304545: the SU UMaNature Confirmed, 2006, PASJ, 58, 383

No. 506 Imada, A., Kubota, K., Kato, T., Nogami, D., Maehara, H., Nakajima, K., Uemura,M., Ishioka, R.

Discovery of a New Dwarf Nova, TSS J022216.4+412259.9: WZ Sge-Type Dwarf NovaBreaking the Shortest Superhump Period Record, 2006, PASJ, 58, L23

No. 507 Isobe, H., Miyagoshi, T., Shibata, K., and Yokoyama, T.

Three-Dimensional Simulation of Solar Emerging Flux Using the Earth Simulator I. Mag-netic Rayleigh-Taylor Instability at the Top of the Emerging Flux as the Origin of Fila-mentary Structure, 2006, PASJ, 52, 423.

No. 508 Kamio, S. and Kurokawa, H.

The relation between Ca bright grains and oscillations in the photosphere, 2006, A&A,450, 351

No. 509 Koide, S., Kudoh, T., Shibata, K.

Jet Formation driven by Expansion of Magnetic Bridges between Ergosphere and Diskaround Rapidly Rotating Black Holes, 2006 Phys. Rev., 74, 44005.

No. 510 Kozu, H., Kitai, R., Brooks, D.H., Kurokawa, H., Yoshimura, K., and Berger, T.E.

Horizontal and Vertical Flow Structure in Emerging Flux Regions, 2006, PSAJ, 58, 407

No. 511 Magara, T.

Dynamic and Topological Features of Photospheric and Coronal Activities Produced byFlux Emergence in the Sun, 2006 ApJ, 653, 1499.

No. 512 Miura, N., Kobayashi, T., Sakuma, R., Kuwamura, S., Baba, N., Hanaoka, Y.,UeNo, S., Kitai, R.

Solar Adaptive Optics System Based on Software Control, 2006, Optical Revies, 13, 338

No. 513 Nagashima, K., and Yokoyama, T.

Statistical Study of the Reconnection Rate in Solar Flares Observed with Yohkoh SXT,2006, ApJ, 647, 654.

No. 514 Nagata, S., Bellot Rubio, L.R., Katsukawa, Y.

Dynamical Properties of Photospheric Flux Tubes at the Footpoints of Hot and CoolCoronal Loops, 2006, ApJ, 638, 539

No. 515 Narukage, N., and Shibata, K.

Statistical Analysis of Reconnection Inflows in Solar Flares Observed with SOHO EIT,2006, ApJ, 637, 1122

76

No. 516 Oka, M., T. Terasawa, Y. Seki, M. Fujimoto, Y. Kasaba, H. Kojima, I. Shinohara,H. Matsui, H. Matsumoto, Y. Saito, and T. Mukai,

Whistler critical Mach number and electron acceleration at the bow shock: Geotail obser-vation, 2006, Geophys. Res. Lett., 33, L24104, doi:10.1029/2006GL028156.

No. 517 Sudo, Y., Baba, N., Miura, N., UeNo, S., and Kitai, R.

Application of self-deconvolution method to shift-and-add solar imaging, 2006, AppliedOptics, 45, 2707.

No. 518 Takeuchi, T. T., Ishii, T. T., Dole, H., Dennefeld, M., Lagache, G., & Puget, J.-L.

The ISO 170um Luminosity Function of Galaxies, 2006, A&A, 448, 525

77

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