国際会議「International CAWSES Symposium」報告
2
0
0
全文
(2)
(3) .
(4)
(5) . t}2 =!~ Px% _P. 2007 10 23 5
(6) . {Q P)E+ -P34 CAWSES. !" #Interna-. S
(7) " #,`Sa (2)
(8) co-chair M$. tional CAWSES Symposium$ %&'()*+. "@)E+2. CAWSES , Climate and Weather of the Sun-. % ,
(9) K@ &LM'*. Earth System -. /0
(10) 1
(11) 2
(12) . "
(13) rStS, (#)*. 345 67 (ICSU)
(14) 489
(15) :;<=. -B2 +,: --. /B2. Scientific Committee on Solar-Terrestrial Physics. # : - .
(16) 2 M. A. Geller. (SCOSTEP) % 2004ῌ2008 >?*"@=34. (Stony Brook Univ.)
(17) 4 -%; SCOSTEP,. ABC DE+ . FG /H. IBC BC. IJI I=K@LM:;
(18). 5.
(19) - . /BC. 0 -. /02 *" N ()O)P. BC/ #d
(20) 0
(21) B. QRST
(22) UVMW* XMY"Z. C$ -1e #:2 21 COE . 6[\]M^*"@)E+ _`Sa, (1). s¡¢ #2
(23) £3¤ 45¤
(24) ¥¦§6$. Solar Influence on Climate -.
(25) 1 [
(26) b. -1e ¨©ª72 21 COE s¡. c2 (2) Space Weather: Science and Applications. ¢ #x /I
(27) W8$ -1e 9#«2. -d
(28) e 5 f 2 (3) Atmospheric Cou-. - 21 COE s¡¢ #. J. pling Processes -ghi2 (4) Space Cli-. /J:I¬® 0
(29) $ -1e ¯;. matology -. /0
(30) jk BC2
(31) l;E+. °2 ±0²BC³´ @µ¶;
(32) ·¸J³¹.
(33) , `Sa (1) m@",. n.
(34) A_')*+ ) % 67. (2) ,. opq CME -rstu. . /HJ /FI 6 %V 6 . v2 Pw
(35) xUV (4) ,. yz{T -|z. % /F5 <h. %
(36) 6. º» 1 292. ¼hº»+
(37) 0. 2008 5 .
(38) ῌ ῍. iC$4 tutorial lecture . j. 5419819k 6
(39) 4789;:;/ G. i4< l$m 94noS. p,q9 =C
(40) $r=/>O 15 s 4 keynote ;< . t56?u4vwMKM. xwI@ f
(41). y/@4564z{|B/. 01
(42) A4BeC3 uv 2. 4A4BeC3 fgT keynote ; </gTw-¸¹!x !yºz. !f} ~4. ~DEF4d IJ. ~GHI^) d K. MxwI@;<0C :>4w J 5 F4J KL;< 45 s j 5?;<M 100 sQ@AB;<M 250 s.
(43) . 0C 5 'NT CAWSES V. . IMO456C3/jP &Q. . !"#$ 376 %&". /0i DERq94JSK&. ! 26 '!#$ 154 ( )* . T/U DE%&9 d8VW%&9. +,-./01 23 4
(44) . X01d%&9. !456. 456<456F4\/]UgTi. 7"456894)*. 1dq9. dY9 Z[9K. : . tutorial lecture keynote. ^4i456< QOT. ;</ 1 =0. :> ?;< 2 =. D ¡¢/!£S ¤R ¥. @AB;< 1 = #C
(45) 0@ADE/ 5 . g y_ `$aQ4¦F/>O 2009 N. F
(46) G HI@'BJK4. %CAWSES _b( §¨ SCOSTEP cd©ª. DLMK,. 4e«#K$ fg456h¬
(47) . 5 FNE #$. / O 4. )* PQ C. Q/iTi . i4j4D. 1 # CRS tutorial lecture
(48). ERq94!£= &K D. K. E<4Ik 60 l; K,. !9T Eugene N. Parker "U. “Hydrodynamics,. Magnetohydrodynamics,. Electric Circuit Analogs” #. and. $VWX. , 7. "#$4DE564Ik 20 \ #K #1 4 . ®S¯mKi ^!. Y%&94Z'4(/
(49) [4. QOTDEῌR<4\ °,U±. \#. ² i³g. ]^)5*+4,-._/ “Early. Japanese Contributions to Space Weather Research”. SCOSTEP `a+4 Marvin A. Geller. !£S <F\ . nop´ y> K ^ . " U “1960 s Advances in Middle Atmosphere. . Research” #[CbC@cB@%&9. #$4-./ i/¶
(50) Q. 01d56423e fgTh4K;</
(51). g. { 101 ». {5¼. ^9qrµ= ^s!"t=¶mr·. 293.
(52)
関連したドキュメント
In this state space model, the stochastic system model is represented by the stochastic Equations (4) and (5) and the probability distributions given in Section (2.3); the
Therefore, when gravity is switched on, the extended momentum space of a point particle is given by the group manifold SL(2, R ) (to be contrasted with the vector space sl(2, R ) in
Arnold This paper deals with recent applications of fractional calculus to dynamical sys- tems in control theory, electrical circuits with fractance, generalized voltage di-
Arnold This paper deals with recent applications of fractional calculus to dynamical sys- tems in control theory, electrical circuits with fractance, generalized voltage di-
Any nonstandard area-minimizing double bubble in H n in which at least one of the enclosed regions is connected consists of a topological sphere intersecting the axis of symmetry
Any nonstandard area-minimizing double bubble in H n in which at least one of the enclosed regions is connected consists of a topological sphere intersecting the axis of symmetry
Any nonstandard area-minimizing double bubble in H n in which at least one of the enclosed regions is connected consists of a topological sphere intersecting the axis of symmetry
Such bounds are of interest because they can be used to improve estimates of volumes of hyperbolic manifolds in much the same way that B¨ or¨ oczky’s bounds [B¨ o1], [B¨ o2] for
