MHD) MHD MHD 1977 MHD ApJ MHD simulation Abstract/Keywords ADS simulation ApJ MHD simulation 1982

Similar documents
8 8 0

(MHD) ( ) MHD 2

erg ( ) 2 ( ) 3 E mag = B2 B L 8π L G 10 5 erg (1) km 3.1

研究成果報告書

,

2015年1月21日CfCAユーザーズミーティング(和田) 非対称電流シートでの 磁気リコネクション XC-Trial, XC-B 和田 智秀1 新田 伸也1 淵田 泰介2 近藤 光志2 1:筑波技術大 2:愛媛大学

本講演の内容 1. はじめに 2. 天体 MHD 現象のおもしろさ 3. 天体 MHD シミュレーションは超困難 4. 天体 MHD シミュレーションの魅力 5. 天体 MHD シミュレーションの魔力 はまると危険 ( 落とし穴の数々 ) 6. むすび : ノーベル賞課題 ( 超難問 ) に挑戦せよ

g µν g µν G µν = 8πG c 4 T µν (1) G µν T µν G c µ ν 0 3 (1) T µν T µν (1) G µν g µν 2 (1) g µν 1 1 描

ohpr.dvi

橡点検記録(集約).PDF

- 1 -


レジャー産業と顧客満足の課題

7-3 2004年新潟県中越地震

untitled

01_教職員.indd


110510_名大HPC(寺田).ppt

Q&A(最終版).PDF

ha ha km2 15cm 5 8ha 30km2 8ha 30km2 4 14

E 1 GeV E 10 GeV 1 2, X X , GeV 10 GeV 1 GeV GeV π

200708_LesHouches_02.ppt

64 3 g=9.85 m/s 2 g=9.791 m/s 2 36, km ( ) 1 () 2 () m/s : : a) b) kg/m kg/m k


NGGAUM_特別対談_再.indd

BC2007_11_ indd



0946: : : :30 UT 1004:30 UT global expansion global expansion pseudo breakup pseudo breakup 3 1: Kotzebue UT [Sh

2015電磁波_歯科医.rtfd

KT

Nosé Hoover 1.2 ( 1) (a) (b) 1:


1 a b cc b * 1 Helioseismology * * r/r r/r a 1.3 FTD 9 11 Ω B ϕ α B p FTD 2 b Ω * 1 r, θ, ϕ ϕ * 2 *

ドコモP-01Hカタログ

NIHSS score p NIHSS score p149 4 p g ml 0.8 g ml D 1 D NIH NIHSS 14 D 0.8 g ml

東海道新幹線でDS



JA2008

.T.C.Y._.E..

Outline I. Introduction: II. Pr 2 Ir 2 O 7 Like-charge attraction III.

1 r 8, , 238 N, Z 28, 50, 82, 126 r cm cm 3 1,000 1 s s slow s 8 s 2 2 s s * 1 * 2 * 3 1 N 50, 82, s * r

<91E F1938C966B95FA8ECB90FC88E397C38B5A8F708A778F7091E589EF8EC08D7388CF88F5837D836A B E696E6464>

( )

-26-

untitled

クレイによる、主婦湿疹のケア

(3)(4) (3)(4)(2) (1) (2) 20 (3)

... 6

untitled

群馬県野球連盟


<82B582DC82CB8E7188E782C48A47967B41342E696E6464>

untitled



裁定審議会における裁定の概要 (平成23年度)


Microsoft Word - 入居のしおり.doc

untitled

和県監査H15港湾.PDF

ESPEC Technical Report 12

syogaku


Taro12-希少樹種.jtd

日本経大論集 第45巻 第1号


untitled

河川砂防技術基準・基本計画編.PDF

4 100g

2

Professional Activities Publications Journal Publications Vice-Chair, Committee on Fluid Structure Interaction, Applied Mechanics Division, ASME Membe

GJG160842_O.QXD

(11-5) Abstract : An ultrasonic air pump utilizing acoustic streaming is discussed and its efficient simulation method using finite element analysis (

工学的な設計のための流れと熱の数値シミュレーション

PowerPoint プレゼンテーション

ssastro2016_shiromizu

6 2 T γ T B (6.4) (6.1) [( d nm + 3 ] 2 nt B )a 3 + nt B da 3 = 0 (6.9) na 3 = T B V 3/2 = T B V γ 1 = const. or T B a 2 = const. (6.10) H 2 = 8π kc2

阪神5年PDF.PDF

12 1



untitled

Microsoft Word - 01_表紙

第4回 小平市の文化振興を考える市民委員会

<4D F736F F D2089AB93EA8CA48F43838C837C815B83675F8FAC97D1>

2

渋谷区耐震改修促進計画

2

Microsoft Word - 第8回問題(3級)


1,000m 875m1 6km

Ⅰ.市区町村事例ヒアリング結果の詳細

一太郎 13/12/11/10/9/8 文書

Microsoft Word - NEWホノルル.docx

私にとっての沖縄と独自性.PDF

00.pdf

Microsoft Word - P01_導水路はいらない!愛知の会 会報11号-1 .docx


Transcription:

MHD) MHD MHD 1977 MHD ApJ MHD simulation Abstract/Keywords 1982 86 5 23 1987 91 57 1992 1996 127 1997 2001 232 ADS simulation ApJ MHD simulation 1982 2001 MHD simulation ApJ 39 ( 71 ) MHD simulation M2 MHD MHD MHD 1997 2001 MHD simulation ApJ simulation MHD

MHD MHD MHD shock MHD vs bulk outflow MHD MHD (Tajima and Shibata 1997)

MHD 100 km 2 14 2 3 / 2 t D = L / η 10 L9 T6 s 300 4 3 / 2 2 9 6 Spitzer η = ηspitzer 10 T6 cm / s, L9 = L /10 cm, T6 = T /10 K MHD t A = L / VA = 10sec t D t A 13 Rm = td / t A = LVA / η 10 2001 = driven reconnection; Sato and Hayashi 1979 Ugai 1982, Yokoyama and Shibata 1994) MHD (Ugai and Tsuda 1977, Ugai 1982, Yokoyama and Shibata 1994) Petschek Sweet-Parker ( 10 4 ) Petschek Petschek-like MHD

MHD MHD MHD ;, Goldreich-Julian density 2 2 1 1 kt 8 T n l mfp = 10 2 cm 6 9 3 n e 10 K 10 cm 10 1 1/ 2 m 10 6 100 10 ivc B T rli = cm eb G K 10 10 3 dive div( VxB / c) 2 3 B V L 9 3 ngj = = 10 cm << 10 7 9 ncorona cm 4πe 4πe 100G 10 cm / s 10 cm 10 12 G 10 5 cm 1 MHD MHD MHD

10 MHD Alfven mode, slow mode, fast mode MHD MHD MHD Balsara 1998, Ryu and Jones 1995, Nakajima and Hanawa 1996, Sano 2000 MHD fast mode s slow mode 2 MHD Alfven mode MHD MHD

MHD MHD MHD MHD MHD CIP CIP-MOCCT CIP CIP (Yabe and Aoki 1991, 1992 1999) CIP Cubic Interpolated Pseudoparticle/Propagation (Yabe et al. 2001) Constrained Interpolation Profile CIP f f + u = 0 t x u= f(x,t)=f( u t, t) a

CIP (a) (b) (c) (b) (d)cip 1999 CIP CIP u= f f + u = 0 t x 3 CIP 2 MHD u= CIP MHD Vlasov

Lax-Wendroff CIP Nakamura et al. 2001 ( 1999 ) MHD MOCCT MHD CIP CIP MHD MOCCT CIP CIP CIP-MOCCT MHD MOCCT MOC Method-Of-Characteristics Stone and Norman 1992 CT Constrained Transport) Evans and Hawley 1988 CT,div B = 0 Alfven Alfven wave Method Of Characteristics=MOC Stone and Norman (1992) MHD MOCCT Stone-Norman MHD ZEUS M. Norman

MHD MOCCT CIP MOCCT Kudoh et al. (1999) 2.5 MHD Kudoh et al. 1998 modified Lax-Wendroff scheme CIP-MOCCT scheme CIP-MOCCT scheme CIP CIP MOCCT MHD

0.01 0.1 CIP MOCCT MOCCT MHD Hawley and Stone 1995 (Clarke 1996) Clarke s MOCCT CMOCCT MHD MHD 5 MHD MHD Tanuma et al. (2001) 2. Shibata and Tanuma (2001 Yokoyama and Shibata (1998, 2001)

Alfven time B L T B 6/7 T 2/7 Shibata and Yokoyama 1999 (Kato et al. 2002, Kudoh et al. 2002, Tomisaka 2002 ) scaling Kudoh et al. 1998, Shibata and Kudoh 1999 for a review ) Koide et al. (2002) Tomisaka(2002) (Sato et al., 2003, in preparation) 10 MHD 0.1 (Hawley et al. 1995, Brandenburg et al. 1995, Matsumoto and Tajima 1995) Machida 2000 3 MHD MHD Sano and Inutsuka (2001) 3D tearing instability MHD additional physics (e.g., heat conduction, cosmic ray,,,) ( MHD

MRI saturation mechanism MHD CIP-MOCCT code MHD e.g., MHD Adaptive mesh refinement MHD Vlasov ADS Balsara, D. (1998) ApJS, 115, 119 Clarke, D. A. (1996) ApJ 457, 291 Evans, C. R. and Hawley, J. F. (1988) ApJ 332, 659 Hawley, J. F. and Stone, J. M. (1995) Comp. Phys, Comm. 89, 127 Koide, S. et al. (2002) Science 295, 1688 Kudoh, T., Matsumoto, R., Shibata, K. (1998) ApJ 508, 186 Kudoh, T., Matsumoto, R., Shibata, K. (1999) Comp. Fluid Dyn. J., 8, 56 Machida, M., Hayashi, M. R. and Matsumoto, R. (2000) ApJ 532, L67 Nakajima, Y. and Hanawa, T. (1996) ApJ 467, 321. Nakamura, T. et al. (2001) J. Comp. Phys. 174, 171 (2001) 77, 948 Ryu, D. and Jones, T. W. (1995) ApJ 442, 228 Sano, T. (2000) Ph. D. Thesis, Univ. of Tokyo Sano, T. and Inutsuka, S. (2001) ApJ 566, 148 Sato, T. and Hayashi, T. (1979) Phys. Fluids, 22, 1189 Shibata, K. and Kudoh, T. (1999) in Proc. Star Formation 1999, p. 263 Shibata, K. and Tanuma, S. (2001) Earth, Planets, and Space 53, 473 Stone, J. M. and Norman, M. L. (1992) ApJS, 80, 791 Tajima, T. and Shibata, K. (1997) Plasma Astrophysics, Addison Wesley Tanuma, S. et al. (2001) ApJ 551, 312 Tomisaka, K. (2002) ApJ 575, 306 Ugai, M. (1982) Phys. Fluids 25, 1027 Ugai, M. and Tsuda, T. (1977) J. Plasma Phys. 17, 337 1999 75 503 Yabe, T. and Aoki (1991) Computer Physics Communications, 66, 219-232 Yabe, T., Xiao, F., and Utsumi, T. (2001) J. Comp. Phys. 169, 556 Yokoyama, T. and Shibata, K. (1994) ApJ 436 197 Yokoyama, T. and Shbata, K. (2001) ApJ 549 1160