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Inoue, Tsuyoshi, Yamazaki, Ryo, Inutsuka, Shu-ichiro (2009) TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM. The Astrophysical Journal, 695 (2). 825-833 doi:10.1088/0004-637x/695/2/825

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Reference TypeJournal (article/letter/editorial)
TitleTURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM
JournalThe Astrophysical Journal
AuthorsInoue, TsuyoshiAuthor
Yamazaki, RyoAuthor
Inutsuka, Shu-ichiroAuthor
Year2009 (April 20)Volume695
Issue2
PublisherIOP Publishing
DOIdoi:10.1088/0004-637x/695/2/825Search in ResearchGate
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Mindat Ref. ID3373009Long-form Identifiermindat:1:5:3373009:7
GUID0
Full ReferenceInoue, Tsuyoshi, Yamazaki, Ryo, Inutsuka, Shu-ichiro (2009) TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM. The Astrophysical Journal, 695 (2). 825-833 doi:10.1088/0004-637x/695/2/825
Plain TextInoue, Tsuyoshi, Yamazaki, Ryo, Inutsuka, Shu-ichiro (2009) TURBULENCE AND MAGNETIC FIELD AMPLIFICATION IN SUPERNOVA REMNANTS: INTERACTIONS BETWEEN A STRONG SHOCK WAVE AND MULTIPHASE INTERSTELLAR MEDIUM. The Astrophysical Journal, 695 (2). 825-833 doi:10.1088/0004-637x/695/2/825
In(2009, April) The Astrophysical Journal Vol. 695 (2) IOP Publishing

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Inoue, Tsuyoshi, Inutsuka, Shu-ichiro (2016) FORMATION OF H i CLOUDS IN SHOCK-COMPRESSED INTERSTELLAR MEDIUM: PHYSICAL ORIGIN OF ANGULAR CORRELATION BETWEEN FILAMENTARY STRUCTURE AND MAGNETIC FIELD. The Astrophysical Journal, 833 (1). 10pp. doi:10.3847/0004-637x/833/1/10
Inoue, Tsuyoshi, Yamazaki, Ryo, Inutsuka, Shu-ichiro, Fukui, Yasuo (2012) TOWARD UNDERSTANDING THE COSMIC-RAY ACCELERATION AT YOUNG SUPERNOVA REMNANTS INTERACTING WITH INTERSTELLAR CLOUDS: POSSIBLE APPLICATIONS TO RX J1713.7–3946. The Astrophysical Journal, 744 (1). 71pp. doi:10.1088/0004-637x/744/1/71
Muto, Takayuki, Inutsuka, Shu-ichiro (2009) ORBITAL EVOLUTION OF A PARTICLE INTERACTING WITH A SINGLE PLANET IN A PROTOPLANETARY DISK. The Astrophysical Journal, 695 (2). 1132-1150 doi:10.1088/0004-637x/695/2/1132
Inoue, Tsuyoshi, Yamazaki, Ryo, Inutsuka, Shu-ichiro (2010) TWO-STEP ACCELERATION MODEL OF COSMIC RAYS AT MIDDLE-AGED SUPERNOVA REMNANTS: UNIVERSALITY IN SECONDARY SHOCKS. The Astrophysical Journal, 723 (1). doi:10.1088/2041-8205/723/1/l108
Roh, Soonyoung, Inutsuka, Shu-ichiro, Inoue, Tsuyoshi (2016) Diffusion of cosmic rays in a multiphase interstellar medium swept-up by a supernova remnant blast wave. Astroparticle Physics, 73. 1-7 doi:10.1016/j.astropartphys.2015.06.001
Takamoto, Makoto, Inoue, Tsuyoshi, Inutsuka, Shu-ichiro (2012) ENHANCED DISSIPATION RATE OF MAGNETIC FIELD IN STRIPED PULSAR WINDS BY THE EFFECT OF TURBULENCE. The Astrophysical Journal, 755 (1). 76pp. doi:10.1088/0004-637x/755/1/76
Iwasaki, Kazunari, Inutsuka, Shu-ichiro (2014) SELF-SUSTAINED TURBULENCE WITHOUT DYNAMICAL FORCING: A TWO-DIMENSIONAL STUDY OF A BISTABLE INTERSTELLAR MEDIUM. The Astrophysical Journal, 784 (2). 115pp. doi:10.1088/0004-637x/784/2/115
Inoue, Tsuyoshi, Inutsuka, Shu-ichiro (2009) TWO-FLUID MAGNETOHYDRODYNAMICS SIMULATIONS OF CONVERGING H I FLOWS IN THE INTERSTELLAR MEDIUM. II. ARE MOLECULAR CLOUDS GENERATED DIRECTLY FROM A WARM NEUTRAL MEDIUM?. The Astrophysical Journal, 704 (1). 161-169 doi:10.1088/0004-637x/704/1/161
Umeda, Takayuki, Yamao, Masahiro, Yamazaki, Ryo (2009) ELECTRON ACCELERATION AT A LOW MACH NUMBER PERPENDICULAR COLLISIONLESS SHOCK. The Astrophysical Journal, 695 (1). 574-579 doi:10.1088/0004-637x/695/1/574
Stroman, Wendy, Pohl, Martin (2009) RADIO POLARIMETRY SIGNATURES OF STRONG MAGNETIC TURBULENCE IN SUPERNOVA REMNANTS. The Astrophysical Journal, 696 (2). 1864-1870 doi:10.1088/0004-637x/696/2/1864
Inoue, Tsuyoshi, Inutsuka, Shu‐ichiro, Koyama, Hiroshi (2006) Structure and Stability of Phase Transition Layers in the Interstellar Medium. The Astrophysical Journal, 652 (2). 1331-1338 doi:10.1086/508334
 
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