2002.1.6$B!!HG(B


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$B=PHG(B

T. Akabane, T. Nakakushi, K. Iwasaki, and S. M. Larson
$B!!(BMartian polar hoods and polar cap in 2001
$B!!(BProc. 34th ISAS Lunar Plan. Symp. PP.21-24, 2001

Asai, A., Ishii, T.T., Kurokawa, H.
$B!!(BPlasma Ejections from a Light Bridge in a Sunspot Umbra
$B!!(B2001, ApJ, 555, L65

Asai, A., Shimojo, M., Isobe, H., Morimoto, T., Yokoyama, T., Shibasaki, K., and Nakajima, H.
$B!!(BPeriodic Acceleration of Electrons in the 1998 November 10 Solar Flare
$B!!(B2001, ApJ, 562, L103

Kurokawa,H., Wang,T and Ishii,T.T.,
$B!!(BEmergence and Drastic Break-down of a Twisted Flux Rope Triggering $B!!(B
$B!!(BStrong Solar Flares in an Active Region NOAA 9026$B!!(B
$B!!(BAstrophys. J. (2002) in press

Shimojo,M., Kurokawa,H., Yoshimura,K,
$B!!(BDynamical Features and Evolutional Characteristics of Brightening
$B!!(BCoronal Loops
$B!!(BSolar Phys.(2002) in press

Nakakushi, T., T. Akabane, K. Iwasaki, and Stephen M. Larson
$B!!(BMars: The cloud effect on the blue clearing in the Syrtis Major region
$B!!(BJ. Geophys. Res., Vol. 106 , No. E3 , p. 5043-5056, 2001

Nakakushi, T., T. Akabane, K. Iwasaki, and Stephen M. Larson
$B!!(BMars: Dissipating behavior of the cloud belt
$B!!(B(submitted to Publ. Astron. Soc. Jpn.)

Takeuchi, A. and Shibata, K.,
$B!!(BMagnetic Reconnection induced by Convective Intensification of
$B!!(BSolar Photospheric Magnetic Fields,
ApJ Let., 546, L73-L76 (2001)

Yokoyama, T., and Shibata, K.,
$B!!(BMagnetohydrodynamic Simulation of a Solar Flare with$B!!(B
$B!!(BChromospheric Evaporation Based on Magnetic Reconnection Model,
$B!!(BApJ, 549, 1160-1174(2001)

Shimojo, M., Shibata, K., Yokoyama, T., and K. Hori,
$B!!(B1D and 2D Pseudo 2D Hydrodynamic Simulations of Solar X-ray Jets,
$B!!(BApJ, 550, 1051-1063 (2001)

Nitta, S., Tanuma,S., Shibata, K., and Maezawa, K.
$B!!(BFast Magnetic Reconnection in Free Space: Self-similar Evolution
$B!!(BProcess,
$B!!(BApJ, 550, 1119-1130 (2001)

Shibata, K. and Tanuma, S.,
$B!!(BPlasmoid-Induced-Reconnection and Fractal Reconnection,
Earth, Planets, Space, 33, 473-482 (2001)

Saito, T., Kudoh, T., and Shibata, K.,
$B!!(BWhat determines the height of spicules ?
I. Alfven wave model and slow wave model,
ApJ, 554, 1151-1158 (2001)

Chen, P. F., Shibata, K., and Yokoyama, T.,
$B!!(BGlobal Destablization due to Localized Reconnection:
$B!!(BA Mechanism for Coronal Mass Ejections,
$B!!(BEarth, Planets, Space, 33, 611-614 (2001)

Takeuchi, A. and Shibata, K.,
$B!!(BSolar Photospheric Magnetic Reconnection,
Earth, Planets, Space, 33, 605-608 (2001)

Yashiro, S. and Shibata, K.,
$B!!(BRelation between Thermal and Magnetic Properties of Active Regions
$B!!(Bas a Probe of Coronal Heating Mechanism,
ApJ, Let. 550, L113-L116 (2001)

M. R. Kundu, A. Nindos, N. Vilmer, K.-L. Klein, K. Shibata, and M. Ohyama,
$B!!(BMetric Radio Emission Associated with X-Ray Plasmoid Ejections,
ApJ, 559, 443-451 (2001)

Nogami, D., Kato, T., Baba, H., Novak, R., Lockley, J.J., Somers, M.
$B!!(BA normal and superoutburst study of the eclipsing SU UMa star:
$B!!(BDV Ursae Majoris
$B!!(B2001, MNRAS, 322, 79

Kato, T., Nogami, D.
$B!!(BOutburst Photometry of DX And
$B!!(B2001, Info. Bull. Var. Stars, No. 5098

Kato, T., Nogami, D., Baba, H.
$B!!(BOutburst Photometry of FX Cep
$B!!(B2001, Info. Bull. Var. Stars, No. 5103

Novak, R., Vanmunster, T., Jensen, L.T., Nogami, D.
$B!!(BThe 1997 Superoutburst of the SU UMa-type Dwarf Nova V2176 Cygni
$B!!(B2001, Info. Bull. Var. Stars, No. 5108

Kato, T., Nogami, D., Lockley, J.J., Somers, M.
$B!!(BUW Tri: Another Likely WZ Sge-type Star
$B!!(B2001, Info. Bull. Var. Stars, No. 5116

Kato, T., Nogami, D., Baba, H., Masuda, S.
$B!!(BOutburst cycle of V363 Lyr
$B!!(B2001, Info. Bull. Var. Stars, No. 5118

Kato, T., Nogami, D., Baba, H.
$B!!(BPhotometry of UZ Tau
$B!!(B2001, Info. Bull. Var. Stars, No. 5121

Kato, T., Nogami, D.
$B!!(BOutbursts of CG Dra
$B!!(B2001, Info. Bull. Var. Stars, No. 5124

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$B!!(BA Deep Dip during an Outburst in the Old Nova, Q Cygni
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Masi, G., Starkey, D., Peitz, J., Martin, B., Baba, H., Sadakane, K.,
Norimoto, Y., Nogami, D., Makita, M.
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$B!!(B2001, IAU Circular, No. 7678

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Nogami, D., Buczynski, D., Baba, H., Kato, T.
$B!!(BThe SU UMa Nature of V630 Cygni
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Kato, T., Matsumoto, K., Nogami, D., Marikawa, K., Kiyota, S.
$B!!(B1998 Superoutburst of the Large-Amplitude SU UMa-Type Dwarf Nova WX Ceti
$B!!(B2001, PASJ, 53, 893

Kato, T., Nogami, D., Baba, H.
$B!!(BThe 1996-1997 Fading of V651 Monocerotis, the Binary Central Star
$B!!(Bof the Planetary Nubula NGC 2346
$B!!(B2001, PASJ, 53, 901

Takeuchi, T.T., Ishii, T.T., Hirashita, H., Yoshikawa, K., Matsuhara,H., Kawara, K., & Okuda, H.
$B!!(BExploring Galaxy Evolution from the Infrared Number Counts and
$B!!(BCosmic Infrared Background
$B!!(B2001, PASJ, 53, 37.

Ishii T T, Inoue K, Kamio S, Sakai K, Watanabe Y, & Kurokawa H
$B!!(BEvolution of H-alpha Fine Loop Structures Observed in a
$B!!(BLong-duration Solar Flare
$B!!(B2001, Advances in Space Research, 26, 1789

Takeuchi, T.T., Kawabe, R., Kohno, K., Nakanishi, K., Ishii, T.T.,Hirashita, H., & Yoshikawa, K.
$B!!(BImpact of Future Submillimeter and Millimeter Large Facilities on the
$B!!(BStudies of Galaxy Formation and Evolution
$B!!(B2001, PASP, 113, 586

Takeuchi, T.T., Ishii, T. T. , Hirashita, H., & Yoshikawa, K.
$B!!(BDusty Era of the Universe: Infrared Galaxy Number Counts and Cosmic Infrared
$B!!(BBackground
$B!!(B2001, in The Physics of Galaxy Formation, ASP Conference Series, 222, 415

Takeuchi, T.T., Hirashita, H., Ishii, T. T. , & Yoshikawa, K.
$B!!!!(BCosmic Star Formation History Inferred from Optical and Far Infrared Observations
$B!!(B2001, in The Birth and Evolution of the Universe,
$B!!(B4th RESCEU International Symposium, 421

Ishii, T. T. , Takeuchi, T.T., & Kurokawa, H.
$B!!(BActive Region Evolutions and Flare Activities: From the Photosphere to the Corona
$B!!(B2001, in Recent Insights into the Physics of the Sun and Heliosphere:
$B!!(BHighlights from SOHO and Other Space Missions,
$B!!(BIAU Symposium 203, 280

Takeuchi, T.T., Hirashita, H., Ishii, T. T. , & Yoshikawa, K.
$B!!(BGalaxy Evolution in the Infrared: Galaxy Number Counts and
$B!!(Bthe Cosmic Infrared Background
$B!!(B2001, in The Extragalactic Background and Its Cosmological Implications,
$B!!(BIAU Symposium 204, 303

$BLn>eBg:n(B
$B!!FMH/E7BN!'(B3m$B$G2?$rA@$&$+!)(B,
$B!!!V5~BgE7J8Bf>-Mh7W2h%o!<%/%7%g%C%W!W=8O?!!(Bpp3-27

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Tanuma, S., Yokoyama, T., Kudoh, T., & Shibata, K.
$B!!(B'Two-Dimensional MHD Numerical Simulations of Magnetic Reconnection
$B!!(BTriggered by a Supernova Shock in Interstellar Medium:
$B!!(BGeneration of X-Ray Gas in Galaxy'
$B!!(B2001, ApJ, 551, pp312-332,

$BED>B=S0l!JL>Bg(BSTE$B8&!K!"2#;31{L@!"9)F#E/MN!J9qN)E7J8Bf!K!" $B!!!VB?CJ3,$N%F%"%j%s%0IT0BDj$K$h$kB.$$<'5$%j%3%M%/%7%g%s$N(B
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$B!!J?@.(B12$BG/EY(BRASC$BEEGH2J3X7W;;5!
Tanuma, S., Yokoyama, T., Kudoh, T., & Shibata, K.
$B!!(B'Three-Dimensional Numerical Magnetohydrodynamic Simulations of
$B!!(BMagnetic Reconnection as the Origin of X-ray Gas in the Galaxy'
$B!!(B2001, New Century of X-ray Astronomy $B=8O?(B pp49-50

Tanuma, S., Yokoyama, T., Kudoh, T., & Shibata, K.
$B!!(B'Three-Dimensional Numerical Magnetohydrodynamic Simulations of
$B!!(BMagnetic Reconnection in the Interstellar Medium'
$B!!(BNumerical Methods for Astrophysical Flows $B=8O?!J0u:~Cf!K(B

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$B $B!!%W%i%:%^3KM;9g3X2q;o(B vol. 77, No.10 (2001) pp.948-994
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$B $B!!%U%l%"$NE}0l%b%G%k! $B!!E7J8650i!"(Bvol. 13, No.5, pp.2-8

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$B!!%U%l%"@1$H7cJQ@1$N(B activity$B!'FC$KB@M[7?3hF0$H$N4XO"$K$D$$$F(B, CD ROM

Proceedings of $B#t(Bhe 2nd SOLAR-B SCIENCE MEETING


K.Shibata
$B!!(BSolar-B science Objectives(Overview of the Mission), pp5-24

H.Kurokawa et al.
$B!!(BTwisted structures of emerging magnetic ropes to cause solar Eruptive phenomena, pp313-327

R.Kitai
$B!!(BRelationship between Solar-B and Ground-Based Observatories, pp403-408

A.Asai et al.
$B!!(BSurges Ejected From the Light Bridge in the Active Region NOAA8971, p439

T.T.Ishii et al.
$B!!(BCharacteristics of Flare-productive Sunspot Group, p441

H.Isobe at al.
$B!!(BReconnection Rate in the Decay Phase of a LDE Flare on 1997 May 12, p443

H.Kozu at al.
$B!!(BConvective Structure Derived From Local Correlation 3D MHD Simulation for Coronal Loop Oscillation
$B!!(Bassociated with Flare, p445


$BJ?@.#1#2G/EY1'ChJ| "$BB@M[8=>]$HCO5e!!!]#2#1@$5*$N(BSpace Weather$B8&5f$rC5$k!](B" $B=8O?(B

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$B!!(BMoreton wave$B$H(BEIT wave, pp123-126

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Tongjiang Wang,Jia-long Wang,Yihua Yan,H.Kurokawa,and K.Shibata
$B!!(BThe Large-Scale Coronal Field Structure for a Helo CME, pp131-134





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$B!!(B1999$BG/(B8$B7n(B11$BF|%H%k%33'4{F|?)4QB,!'5~ETBg3X%A!<%`7k2LJs9p(B

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$B!!(BReconnection inflow velocity$B$H%3%m%J<'>l6/EY$N4V@\E*F3=P(B

$B1RF#!!LP!"0kItMNL@!"@.1FE5G7!"@u0f!!Jb!"?9K\B@O:!"!"KL0fNi;0O:(B
$B!!(BMoreton wave$B$H(BEIT wave

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$B!!EEGH$*$h$S9E(BX$B@~$G$H$i$($k%U%l%"$NHsG.E*N3;R2CB.(B

Tongjiang Wang,Jia-long Wang,Yihua Yan,H.Kurokawa,and K.Shibata
$B!!(BThe Large-Scale Coronal Field Structure for a Helo CME


$BKgJ}4uK>652q9V1i2q!JKgJ}!K(B $B#27n#2#5F|(B

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$B $B!!!VE7BN<'5$N.BN8=>]!W(B


New Century of X-ray Astronomy$B!J2#IM!K#37n#6!<#8F|(B

Tanuma, S., Yokoyama, T., Kudoh, T., & Shibata, K. 2001,
$B!!(B'Three-Dimensional Numerical Magnetohydrodynamic Simulations of
$B!!(BMagnetic Reconnection as the Origin of X-ray Gas in the Galaxy'


$BJ?@.(B12$BG/EY(BRASC$BEEGH2J3X7W;;5!
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Seminar at Dept. Astron., Nanjing University$B!!(B(Nanjing, China)$B!!#37n#8F|!]#9F|(B

Shibata K.
$B!!(B``Solar and Stellar Flares''
$B!!(B``Astrophysical Jets''


$BB@M[7w%7%s%]%8%&%`!JL>BgEl;3CO6h!"L>8E20!K!!#37n#1#4F|(B

$B $B!!(B``Generation of Alfven Waves by Magnetic Reconnection$B!!(Band Coronal Heating''


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$B@P0f5.;R!"9u2O9(4k!"KL0fNi;0O:!J5~BgM}!K(B
$B!!(BFlare Activity in Emerging Flux Regions in the Active Region NOAA 9236

T.Wang$B!"(BH.Kurokawa$B!"(BT.T.Ishii$B!J5~BgM}!K!"(BR.Shine$B!J(BLockheed Solar Labs$B!K(B
$B!!(BThe Evidence for Kink Instablity to a $B&D(B-spot Collapse

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$B $B!!!VB@M[$N3hF08=>]$H1'ChE75$!W(B


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$B=);39,;R(B
$B!!HtBM!&2V;3E7J8Bf$K$*$1$k#H&A%U%l%"4QB,$NJs9p(B


American Geophysical Union 2001 Spring Meeting$B!!(B(Boston, Massachusetts$B!K(B
29 May - June 2

A. Takeda (SPRC/ISAS), H. Kurokawa, R. Kitai, and K. Ishiura (Kwasan and$B!!(BHida Observatories, Kyoto Univ.)
$B!!(BDistribution of the Green- and Red-Line Coronal Emissions and Their Contribution to the K-Corona


$BCO5eOG@12J3X4XO"3X2q(B 2001$BG/9gF1Bg2q(B($BEl5~%*%j%s%T%C%/%;%s%?!<(B) 6$B7n(B 4$BF|(B - 8$BF|(B

$B@u0f(B $BJb!"0kIt(B $BMNL@!"(B $B?9K\(B $BB@O:(B $B$[$+(B
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$B0kIt(B $BMNL@!" $B!!!VB@M[%3%m%J$N%"!<%1!<%I7A@.$K$*$1$k(Bdawn-dusk asymmetry$B!W(B

$B?9K\(B $BB@O:(B
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$B5~BgE7J8Bf>-Mh7W2h%o!<%/%7%g%C%W(B $B!JHtBME7J8Bf!K(B 6$B7n(B9$BF|(B

$BLn>eBg:n(B
$B!!FMH/E7BN!'(B3m$B$G2?$rA@$&$+!)(B


Infrared and Submillimeter Space Astronomy: An International Colloquium
to Honor the Memory of Guy Serra $B!!(BToulouse (France)$B!!(B6$B7n(B11$BF|(B--13$BF|(B

Ishii, T. T., Takeuchi, T.T., & Sohn, J-J
$B!!(BInfrared Number Count Model and Estimated Source Confusion Limits


$BCO5e%7%_%e%l!<%?MxMQ8!F$2q!J3$MN2J3X8&5f%;%s%?!
$B $B!!!VB@M[%U%l%"8=>]$NBg5,LO?tCM7W;;!W(B


CEDAR-SCOSTEP meeting, 10th STP Symposium (Longmont, Colorado, USA) $B!!#67n#1#7F|(B

Shibata$B!!(BK.
$B!!(B``Unified View of Solar Flares and Coronal Mass Ejections''


SHINE meeting (Snowmass, Colorado, USA)$B!!#67n#1#8F|(B

Shibata$B!!(BK.
$B!!(B``Plasmoid-Induced-Reconnection Model for Solar Flares and
$B!!(BCoronal Mass Ejections''


1st Korean Astrophysics Workshop on$B!!(B"Numerical Methods for Astrophysical Flows"
(Pusan, Korea)$B!!#67n#2#6!]#2#9F|(B

Shibata$B!!(BK.
$B!!(B``MHD code: applications''
$B!!(B``Magnetic Reconnection and Solar/Stellar Flares''

Isobe, H., Yokoyama, T., and Shibata, K.
$B!!(B"Numerical Simulation of a Protostellar Flare Loop between the Core and Disk"

Tanuma, S., Yokoyama, T., Kudoh, T., & Shibata, K.,
$B!!(B'Three-Dimensional Numerical Magnetohydrodynamic Simulations of
$B!!(BMagnetic Reconnection in the Interstellar Medium'


$B86;RNO8&5f=j7W;;!&@hC<>pJs6&F1MxMQ%;%s%?!
$B $B!!!VB@M[%U%l%"8=>]$NBg5,LO?tCM7W;;!W(B


2001$BG/EY(B $BE7J8!&E7BNJ*M}
$BCf6z9';V!J2V;3E7J8Bf!K!"@V1)FA1Q!JHtBME7J8Bf!K!"4d:j63Je!J5~ET3X1`Bg!K!"(BStephen M.Larson$B!J(BLPL/$B%"%j%>%JBg!K(B
$B!!(B2001$BG/$N4QB,$+$iF@$i$l$?2P@15$8u>uBV$NJs9p(B

$B $B!!!VEA$($?$$E7J83X!&EA$($F$[$7$$E7J83X!W!J0&CN650iBgBt$5$s$H$NBPCL!K(B

$BLn>eBg:n(B
$B!!%U%l%"@1$H7cJQ@1$N(B activity$B!'FC$KB@M[7?3hF0$H$N4XO"$K$D$$$F(B($B>7BT9V1i(B)


The Physics of Cataclysmic Variables and Related Objects
(Goettingen, Germany) 8$B7n(B5-10$BF|(B

Nogami, D., Beuermann, K., Gaensicke, B.T.
$B!!(BOn the magnetic fields in the polar UZ Fornacis

Gaensicke, B.T., Hagen, H.-J., Kube, J., Schwarz, R., Staude, A.,
Nogami, D., Engels, D.
$B!!(BHS 0455+83: A new eclipsing novalike variable


$BBh(B34$B2s7n!&OG@1%7%s%]%8%&%`!JAjLO86!K!!(B8$B7n(B6-8$BF|(B

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$B!!(BPreliminary analyses of the Martian aphelion cloud belt: 2001 observations


$B9qN)E7J8BfLnJU;3EEGH4QB,=jFCJL8x3+!&9V1i2q!JLnJU;3!K!!#87n#2#5F|(B

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$B!!!V%I!<%`%l%9K>1s6@@)8f$N<+F02=!W(B

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$B!!B@M[%U%l%"$H%,%s%^@~%P!<%9%H(B

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$B!!(BMartian cloud belt in autumn:2001 observations

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$B!!#1#9#9#2G/#1#17n#2F|$N(BX$B#9%U%l%"$K$*$1$k(Bpost-flare loop$B$NHy:Y9=B$$N;~4VH/E8(B

$B@P0f5.;R!"9u2O9(4k!"KL0fNi;0O:!J5~BgM}!K(B
$B!!(BPre-flare Activities in the Active Region NOAA 9236

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$B!!#2#0#0#1G/#47n#1#0F|$K5/$-$?(BX2$B%/%i%9%U%l%"$N9E(BX$B@~J|
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$B!!(BHot and Cool Plasma Ejections from Solar Flares on Nov. 24,2000

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$B!!#2#0#0#1G/#47n#1#0F|$N%U%l%"$K$*$1$k!"HsG.E*N3;R$N;~4VJQ2=$N2r@O!J#1!K!'(BH$B&A%+!<%M%k$N%i%$%H%+!<%V(B

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$B!!#2#0#0#1G/#47n#1#0F|$N%U%(%"$K$*$1$k!"HsG.E*N3;R$N;~4VJQ2=$N2r@O!J#2!K!'(BTwo-Ribbon Flare$B$NFbIt9=B$(B

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D.H.Brook$B#s(B(Kwasan and Hida Observatories,Kyoto University)$B!"(BH.Kurokawa(Kwasan and Hida Observatories,Kyoto University)$B!"(BK.Yoshimura(Institute of Space and Astronautical Science)$B!"!!(BT.E.Berger(Lockheed Martin Solar and Astrophysics Lab.$B!"(BPaloAlto,USA)
$B!!(BA study of a solar active region abserved by the La Palma SVST

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