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    <title>Space and Earth System Modeling Research Lab. Unit</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/" />
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    <id>tag:www.jamstec.go.jp,2008-12-24:/less/space_earth/en//3</id>
    <updated>2009-06-19T13:43:11Z</updated>
    <subtitle>Space and Earth System Modeling Research Lab. Unit studies the complicated interaction between the different layers of the Earth system in terms of the state-of-the-art numerical simulations, the observations and the experiments, aiming at understanding the mechanism of the large-scale variations of the earth system.</subtitle>
    <generator uri="http://www.sixapart.com/movabletype/">Movable Type Commercial 4.23-ja</generator>

<entry>
    <title>Gallary</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/gallery/archives.html" />
    <id>tag:hsrptest.yes.jamstec.go.jp,2009:/hsrp/en//3.147</id>

    <published>2009-06-15T06:14:15Z</published>
    <updated>2009-06-19T13:43:11Z</updated>

    <summary> [&#8593; click the figure to see the movie ] Results of MHD simulation of CME. The sphere shows the surface of the Sun (colors: magnetic field) and tubes displays magnetic field lines. [&#8593; click...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
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        <![CDATA[ <a href="/jswm/ja/movies/CME.html" target="_balnk" title="CME"><img src="/hsrp/ja/assets_c/2009/02/cme-thumb-450x210-185.jpg" width="450" height="210" border="0" alt="" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 5px;" /></a><small><strong>[&#8593; click the figure to see the movie ]</strong></small>
Results of MHD simulation of CME. The sphere shows the surface of the Sun (colors: magnetic field) and tubes displays magnetic field lines.
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<a href="/hsrp/ja/movies/cloud.html" target="_balnk"  title="Cloud formation and rainfall simulation"><img src="/hsrp/ja/assets_c/2009/02/cloud1-thumb-450x252-69.gif" width="450" height="252" alt="cloud1.gif" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 20px;" /></a><small><strong>[&#8593; click the figure to see the movie ]</strong></small>
Cloud formation and rainfall simulated by the coupled model of SDM and non-hydrostatic model. 
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<a href="/hsrp/ja/movies/cloud3d.html" target="_balnk"  title="Cloud formation and rainfall simulation"><img src="/hsrp/ja/assets_c/2009/02/cloud3d-thumb-450x476-206.gif" width="450" height="476" border="0" alt="" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 5px;" /></a><small><strong>[&#8593; click the figure to see the movie ]</strong></small>
Cloud formation and rainfall simulated by the coupled model of SDM and non-hydrostatic model. 
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<a href="/hsrp/en/images/gallary/homogeneous.jpg" rel="mediabox[600 670]" title=""><img src="/hsrp/ja/assets_c/2009/02/Unknown-thumb-450x502-258.gif" width="450" height="502" border="0" alt="" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 5px;" /></a>We have applied our interlocked plasma simulation model to the shock problem in the space plasma. In the area of 0 to 10,000 in X axis, the fluid model is performed. And in the area of 10,000 to 15,000, the particle model is performed. Then both models are self-consistently connected. We can see the physics in the extended area with the detailed physics around the shock transition layer.
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<a href="/hsrp/ja/movies/H2o.html" target="_balnk" title="Homogeneous vapor-liquid nucleation of water"><img src="/hsrp/ja/assets_c/2009/02/nucl-thumb-450x451-209.gif" width="450" height="451" border="0" alt="nucl.gif" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 5px;" /></a><small><strong>[&#8593; click the figure to see the movie ]</strong></small>
Homogeneous vapor-liquid nucleation of water. 
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    </content>
</entry>

<entry>
    <title>Publication</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/publication/publication.html" />
    <id>tag:210.251.87.117,2009:/hsrp/en//3.102</id>

    <published>2009-02-06T14:30:23Z</published>
    <updated>2009-02-10T13:30:17Z</updated>

    <summary><![CDATA[Refereed Papers 2009S. Hirose, J. H. Krolik, and O. M. Blaes, &quot;Radiation-dominated Accretion Disks Are Thermally Stable&quot;, Astrophys. J., 691, 16-31, (2009). K. Nishida, M. Shimizu, D. Shiota...]]></summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Publication" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<table border="0" cellspacing="2" cellpadding="4" bgcolor="#e7f4f4" width="100%"><tr><td valign="top"><strong>Refereed Papers</strong></td></tr></table>

<p><br />
<strong>2009</strong><ul><li>S. Hirose, J. H. Krolik, and O. M. Blaes, &quot;Radiation-dominated Accretion Disks Are Thermally Stable&quot;, Astrophys. J., 691, 16-31, (2009).</li></p>

<p><li>K. Nishida, M. Shimizu, D. Shiota, H. Takasaki, T. Magara, and K. Shibata, <a href="http://adsabs.harvard.edu/abs/2009ApJ...690..748N" target="_blank">&quot;Numerical examination of plasmoid-induced reconnection model for solar flares: the relation between plasmoid velocity and reconnection rate</a>, The Astrophysical Journal, 690, 748-757, (2009).</li><br />
</ul></p>

<p><br />
<strong>2008</strong><ul><li>P. Antolin, K. Shibata, T. Kudoh, D. Shiota, and D. Brooks, <a href="http://adsabs.harvard.edu/abs/2008ApJ...688..669A" target="_blank">&quot;Predicting Observational Signatures of Coronal Heating by Alfven Waves and Nanoflares&quot;</a>, The Astrophysical Journal, Volume 688, Issue 1, pp. 669-682, (2008).</li></p>

<p><li>Hiroki Hasegawa, Seiji Ishiguro, and Masao Okamoto, <a href="http://springerlink.com/content/71782n241548231v/?p=63f20b072cdf4d4299fb1f6abfa22b73&amp;pi=32" target="_blank">&quot;Distributed Parallelization of Exact Charge Conservative Particle Simulation Code by High Performance Fortran&quot;</a>, Lecture Notes in Computer Science, 4759, 358-364 (2008).</li></p>

<p><li>S. Inoue, K. Kusano, S. Masuda, T. Miyoshi, T. Yamamoto, T. Magara, S. Tsuneta, T. Sakurai, and T. Yokoyama, &quot;Three-Dimensional Structure Analysis of Coronal Magnetic Field in AR NOAA10930 Based on Vector Magnetogram Observation with Hinode/SOT&quot;, First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity College Dublin, Dublin, Ireland. Edited by Sarah A. Matthews, John M. Davis, and Louise K. Harra. San Francisco: Astronomical Society of the Pacific, p.110, (2008).</li></p>

<p><li>Yoji Kawamura, Hiroya Nakao, Kensuke Arai, Hiroshi Kori, and Yoshiki Kuramoto, <a href="http://link.aps.org/abstract/PRL/v101/e024101" target="_blank">&quot;Collective phase sensitivity&quot;</a>, Phys. Rev. Lett. 101, 024101 (2008).</li></p>

<p><li>Akio Kawano, and Gia G. Maisuradze, <a href="http://www.amsi.ge/jbpc/10808/10803.html" target="_blank">&quot;Interpolated moving least-squares methods for fitting potential energy surfaces: analysis of an application to a five-atom molecule&quot;</a>, J. Biol. Phys. Chem. 8, 17-21 (2008).</li></p>

<p><br />
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<p><br />
<li>Takuma Matumoto, Reizaburo Kitai, Kazunari Shibata, Kenichi Otsuji, Takuya Naruse, Daikou Shiota, Hiroyuki Takasaki, <a href="http://adsabs.harvard.edu/abs/2008PASJ...60...95M" target="_blank">&quot;Height dependence of the gas flows in an Ellerman bomb&quot;</a>, Publications of the Astronomical Society of Japan, 60, 95-102, (2008).</li></p>

<p><li>T. Miyoshi and K. Kusano, &quot;Robust and Efficient Riemann Solvers for MHD&quot;, ASP Conference Series, Vol. 385, NUMERICAL MODELING OF SPACE PLASMA FLOWS / ASTRONUM-2007, eds. Nikolai V. Pogorelov, Edouard Audit, and Gary P. Zank, 279-284 (2008).</li></p>

<p><li>C. J. Schrijver, M. L. DeRosa, T. Metcalf, G. Barnes, B. Lites, T. Tarbell, J. McTiernan, G. Valori, T. Wiegelmann, M. S. Wheatland, T. Amari, G. Aulanier, P. D&#233;moulin, M. Fuhrmann, K. Kusano, S. R&#233;gnier, and J. K. Thalmann, &quot;Nonlinear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection&quot;, Astrophys. J. 675, 1637-1644 (2008).</li></p>

<p><li>M. Shimizu, K. Nishida, H. Takasaki, D. Shiota, T. Magara, and K. Shibata, <a href="http://adsabs.harvard.edu/abs/2008ApJ...683L.203S" target="_blank">&quot;The Correlation among the Rise Velocity of a Soft X-Ray Loop, the Ejection Velocity of a Plasmoid, and the Height above the Loop Top of the Hard X-Ray Source in Masuda-Type Flares, and Its Interpretation Based on the Reconnection Model of Flares&quot;</a>, The Astrophysical Journal Letters, Volume 683, Issue 2, pp. L203-L206, (2008).</li></p>

<p><li>Daikou Shiota, Kanya Kusano, Takahiro Miyoshi, Noriaki Nishikawa, Kazunari Shibata, <a href="http://adsabs.harvard.edu/abs/2008JGRA..11303S05S" target="_blank">&quot;A Quantitative MHD Study of the Relation among Arcade Shearing, Flux Rope Formation, and Eruption due to the Tearing Instability&quot;</a>, the Journal of Geophysical Research, 113, A03S05, (2008).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;Multi-physics Plasma Simulation by the Interlocking of Two Different Hybrid Models&quot;, ASP Conference Series, Vol. 385, NUMERICAL MODELING OF SPACE PLASMA FLOWS / ASTRONUM-2007, eds. Nikolai V. Pogorelov, Edouard Audit, and Gary P. Zank, 228-236, (2008).</li></ul></p>

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<p><br />
<strong>2007</strong><ul><li>O. M. Blaes, S. Hirose, and J. H. Krolik, Surface Structure in an Accretion Disk Annulus with Comparable Radiation and Gas Pressure, Astrophys. J., 664, 1057-1071, (2007).</li></p>

<p><li>Yoji Kawamura, <a href="http://link.aps.org/abstract/PRE/v76/e047201" target="_blank">&quot;Hole structures in nonlocally coupled noisy phase oscillators&quot;</a>, Phys. Rev. E 76, 047201 (2007).</li></p>

<p><li>J. H. Krolik, S. Hirose, and O. M. Blaes, Thermodynamics of an Accretion Disk Annulus with Comparable Radiation and Gas Pressure,Astrophys. J., 664, 1045-1056, (2007).</li></p>

<p><li>K. Kusano, &quot;Simulation Study of Transition Process from Long-Lived Sigmoid to Flare Eruption&quot;, ASP Conference Series, Vol. CS 369, NEW SOLAR PHYSICS WITH SOLAR-B MISSION, The Sixth Solar-B Science Meeting, eds. Kazunari Shibata, Shin'ichi Nagata and Takashi Sakurai, 469-476 (2007).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;Multi-scale Plasma Simulation by the Interlocking of Magnetohydrodynamic Model and Particle-in-Cell Kinetic Model&quot;, J. Comput. Phys. 227, 1340-1352, (2007).</li></p>

<p><li>Osamu Takahashi, Takayuki Matsui, Akio Kawano, Kiyohiko Tabayashi, Katsuyoshi Yamasaki, <a href="http://linkinghub.elsevier.com/retrieve/pii/S0166128006008566" target="_blank">&quot;Systematics of the gradient on the resonant core-hole state&quot;</a>, J. Mol. Struct.: THEOCHEM. 808, 35-40 (2007).</li></p>

<p><li>B. T. Welsch, W. P. Abbett, M. L. DeRosa, G. H. Fisher, M. K. Georgoulis, K. Kusano, D. W. Longcope, B. Ravindra, and P. W. Schuck, &quot;Tests and Comparisons of Velocity Inversion Techniques&quot;, Astrophys. J. 670, 1434-1452 (2007).</li></ul></p>

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<p><strong>2006</strong><ul><br />
<li>O. M. Blaes, S. W. Davis, S. Hirose, J. H. Krolik, and J. M. Stone, &quot;Magnetic Pressure Support and Accretion Disk Spectra&quot;, Astrophys. J., 645, 1402-1407, (2006).</li></p>

<p><li>Hiroki Hasegawa, Seiji Ishiguro, and Masao Okamoto, <a href="http://www.journals.cup.org/action/displayAbstract?fromPage=online&amp;aid=602696&amp;fulltextType=RA&amp;fileId=S0022377806005344" target="_blank">&quot;Particle Acceleration by a Large Amplitude Wave Associated with an Ion Beam in a Magnetized Plasma&quot;</a>, J. Plasma Phys., 72, 941-944 (2006).</li></p>

<p><li>S. Hirose, J. H. Krolik, and J. M. Stone, &quot;Vertical Structure of Gas Pressure-Dominated Accretion Disks with Local Dissipation of Turbulence and Radiative Transport&quot;, Astrophys. J., 640, 901-917, (2006).</li></p>

<p><li>Seiji Ishiguro and Hiroki Hasegawa, <a href="http://www.journals.cup.org/action/displayAbstract?fromPage=online&amp;aid=603224&amp;fulltextType=RA&amp;fileId=S0022377806006003" target="_blank">&quot;Three-Dimensional Particle-In-Cell Simulation of Scrape-off-Layer Plasmas&quot;</a>, J. Plasma Phys., 72, 1233-1237 (2006).</li></p>

<p><li>Akio Kawano and Gia G. Maisuradze, <a href="http://www.amsi.ge/jbpc/10606/10607.html" target="_blank">&quot;Interpolated moving least-squares methods for fitting potential energy surfaces: the dependence on coordinate systems for six-dimensional applications&quot;</a>, J. Biol. Phys. Chem. 6, 37-44 (2006).</li></p>

<p><li>Akio Kawano and Gia G. Maisuradze, <a href="http://www.amsi.ge/jbpc/20606/20607.html" target="_blank">&quot;Reducing the computational cost of ab initio potential energy calculations by using a dual-level approach&quot;</a>, J. Biol. Phys. Chem. 6, 83-89 (2006).</li></p>

<p><li>Akio Kawano, Igor V. Tokmakov, Donald L. Thompson, Albert F. Wagner, and Michael Minkoff, <a href="http://link.aip.org/link/?JCPSA6/124/054105/1" target="_blank">&quot;Interpolating moving least-square methods for fitting potential energy surfaces: Further improvement of efficiency via cutoff strategies&quot;</a>, J. Chem. Phys. 124, 054105 (2006).</li></p>

<p><li>Yoshiki Kuramoto, Shin-ichiro Shima, Dorjsuren Battogtokh, and Yuri Shiogai, &quot;Mean-Field Theory Revives in Self-Oscillatory Fields with Non-Local Coupling&quot; Prog. Theor. Phys. Suppl., 161, pp. 127-143 (2006).</li></p>

<p><li>Yukiharu Ohsawa, Ken Kato, and Hiroki Hasegawa, <a href="http://www.journals.cup.org/action/displayAbstract?fromPage=online&amp;aid=602664&amp;fulltextType=RA&amp;fileId=S0022377806005307" target="_blank">&quot;Simulation Studies of Positron Acceleration by a Shock Wave&quot;</a>, J. Plasma Phys., 72, 919-923 (2006).</li><br />
</ul></p>

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<p><strong>2005</strong><ul><li>Hiroki Hasegawa, Seiji Ishiguro, and Masao Okamoto, <a href="http://www.jstage.jst.go.jp/article/ipsjdc/1/0/1_634/_article" target="_blank">&quot;Development of the Efficient Electromagnetic Particle Simulation Code with High Performance Fortran on a Vector-Parallel Supercomputer&quot;</a>, IPSJ Trans. on ACS, 46 No.SIG16 (ACS12), 144-152 (2005); IPSJ Digital Courier, 1, 634-642 (2005).</li></p>

<p><li>Hiroki Hasegawa, Ken Kato, and Yukiharu Ohsawa, <a href="http://scitation.aip.org/getabs/servlet/GetabsServlet?prog=normal&amp;id=PHPAEN000012000008082306000001&amp;idtype=cvips&amp;gifs=yes" target="_blank">&quot;Persistent Acceleration of Positrons in a Nonstationary Shock Wave&quot;</a>, Phys. Plasmas, 12, 082306-1-082306-6 (2005).</li><br />
</ul></p>

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<p><br />
<table border="0" cellspacing="2" cellpadding="4" bgcolor="#e7f4f4" width="100%"><tr><td valign="top"><strong>Non-refereed Papers</strong></td></tr></table></p>

<p><br />
<strong>2008</strong><ul><li>Kanya Kusano, Shigenobu Hirose, Tooru Sugiyama, Akio Kawano, Shin-ichiro Shima, Hiroki Hasegawa, Daikou Shiota, and Satoshi Inoue, <a href="http://www.jamstec.go.jp/esc/publication/annual/annual2007/pdf/2project/chapter2/129kusano.pdf" target="_blank">&quot;Development of Macro-Micro Interaction Simulation Algorithm&quot;</a>, Annual Report of the Earth Simulator Center April 2007 - March 2008, 129 (2008).</li></p>

<p><li>S. Shima, &quot;Estimation of the Computational Cost of Super-Droplet Method&quot;, RIMS K&ocirc;ky&ucirc;roku 1606, pp.110-118 (2008).</li><br />
</ul></p>

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<p><strong>2007</strong><ul><li>Kanya Kusano, Shigenobu Hirose, Tooru Sugiyama, Akio Kawano, Shin-ichiro Shima, Hiroki Hasegawa, and Daikou Shiota, <a href="http://www.jamstec.go.jp/esc/publication/annual/annual2006/pdf/3project/chapter2/131kusano.pdf" target="_blank">&quot;Development of Macro-Micro Interaction Simulation Algorithm&quot;</a>, Annual Report of the Earth Simulator Center April 2006 - March 2007, 131 (2007).</li><br />
</ul></p>

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<p><strong>2006</strong><ul><li>Kanya Kusano, Shigenobu Hirose, Akio Kawano, Shin-ichiro Shima, and Tohru Sugiyama, <a href="http://www.jamstec.go.jp/esc/publication/annual/annual2005/pdf/P153_Kusano.pdf" target="_blank">&quot;Development of Macro-Micro Interaction Simulation Algorithm&quot;</a>, Annual Report of the Earth Simulator Center April 2005 - March 2006, 153 (2006).</li><br />
</ul></p>

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<p><strong>2005</strong><ul><li>Hiroki Hasegawa, Seiji Ishiguro, and Masao Okamoto, &quot;Development of Exact Charge Conservative Particle Simulation Code with High Performance Fortran&quot;, Annual Report of NIFS, April 2004 &#8211; March 2005, 364 (2005).</li></p>

<p><li>Yukiharu Ohsawa, Mieko Toida, Ken Kato, Masatoshi Sato, Seiji Ishiguro, Hiroki Hasegawa, and Shunsuke Usami, &quot;Self-Organization of Large-Amplitude Waves and Associated Particle Acceleration&quot;, Annual Report of NIFS, April 2004 &#8211; March 2005, 359 (2005).</li></p>

<p><li>Kunihiko Watanabe, Tohru Sugiyama, Akira Kageyama, Kanya Kusano, and Nobuaki Ohno, <a href="http://www.jamstec.go.jp/esc/publication/annual/annual2004/pdf/3project/chapter3/2watanabe.pdf" target="_blank">&quot;Development of Micro-Macro Interaction Simulation Algorithm&quot;</a>, Annual Report of the Earth Simulator Center April 2004 - March 2005, 151 (2005).</li><br />
</ul></p>

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<p><br />
<table border="0" cellspacing="2" cellpadding="4" bgcolor="#e7f4f4" width="100%"><tr><td valign="top"><strong>Conference Presentations (International)</strong></td></tr></table></p>

<p><br />
<strong>2009</strong><ul><li>T. Sugiyama and K. Kusano, &quot;MHD-PIC interlocked simulation model in space plasma&quot;, Voyagers in the Heliosheath (Invited), Hawaii, USA (Jan. 11, 2009).</li><br />
</ul></p>

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<p><strong>2008</strong><ul><li>T. Sugiyama and K. Kusano, &quot;MHD-PIC interlocked simulation model in space plasma&quot;, AGU Fall Meeting 2008, San Francisco, USA (Dec. 18, 2008).</li></p>

<p><li>S. Inoue, D. Shiota, K. Kusano, E. Asano, T. Matsumoto, R. Kataoka, T. Magara, T. Miyoshi, T. Yamamoto, T. Ogino, and K. Shibata, &quot;Three-Dimensional Magnetic Topology in the AR 10930 Based on Non-Linear Force-Free Modeling&quot;, AGU FALL Meeging 2008, San Francisco, USA (Dec. 15-19, 2008).</li></p>

<p><li>D. Shiota, K. Kusano, T. Miyoshi, and K. Shibata, &quot;Launching Process of Coronal Mass Ejections&quot;, AGU FALL Meeging 2008, San Francisco, USA (Dec. 15-19, 2008).</li></p>

<p><li>K. Kusano, &quot;Toward the holistic modeling of solar-cosmic and terrestrial environment system&quot;, Meeting International Workshop on Variabilities of Solar-Cosmic and Terrestrial Environment, Yokohama, Japan (Dec. 4-6, 2008).</li></p>

<p><li>Shin-ichiro Shima, &quot;How to resolve maritime clouds using super droplet method&quot;, International Workshop on Variabilities of Solar-Cosmic and Terrestrial Environment, Yokohama, Japan, (Dec. 4, 2008).</li></p>

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<p><br />
<li>K. Kusano, D. Shiota, S. Inoue, Kataoka, R., Miyoshi. T., Magara, T., Asano, E., Matsumato, T., Yamamoto, T.,Ogino, T., and K. Shibata, &quot;Multi-scale Modeling of Solar Terrestrial Environment System&quot;, International Symposium: Fifty Years after IGY: Modern Information Technologies and Earth and Solar Sciences, Tsukuba, Japan (Nov. 10-13, 2008).</li></p>

<p><li>K. Kusano, &quot;Data-Driven Simulation of Solar Eruption&quot;, Meeting Workshop on Space Weather Modeling, Daejeon, Korea (Oct. 16-17, 2008).</li></p>

<p><li>S. Inoue, D. Shiota, K. Kusano, E. Asano, T. Matsumoto, R. Kataoka, T. Magara, T. Miyoshi, T. Yamamoto, T. Ogino, and K. Shibata, &quot;Data-Driven Interlocked Modeling of the Sun-Earth System&quot;, A preliminary Study on Numerical Modeling for Space Weather, Daejeon, Korea (Sep. 25, 2008).</li></p>

<p><li>K. Shibata, K. Kusano, D. Shiota, S. Inoue, Asano, E., Matsumoto, T., Kataoka, R., Miyoshi, T., Ogino, T. and the Space Weather Modeling Team, &quot;Weather Modeling of the Solar Terrestrial Connection Event in December 2006: From the Sun to Interplanetary Space&quot;, IAU sympo. 257 Universal Heliophysical Processes, Ioannina, Greece (Sep. 15-19, 2008).</li></p>

<p><li>H. Hasegawa, T. Sugiyama, A. Kageyama, S. Hirose, K. Kusano, and T. Sato, &quot;Effect of Microscopic Instability on Quiet Auroral Arc Formation&quot;, ICPP2008: International Congress on Plasma Physics, Fukuoka, Japan (Sep. 8-12, 2008).</li></p>

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<p><br />
<li>K. Kusano, D. Shiota, S. Inoue, R. Kataoka, E. Asano, T. Matsumato, and K. Shibata, &quot;STUDY OF THE INITIATION MECHANISM AND THE PREDICTABILITY OF SOLAR ERUPTION BASED ON DATA-DRIVEN SIMULATION&quot;, ICPP2008: International Congress on Plasma Physics, Fukuoka, Japan (Sep. 8-12, 2008).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;Magnetohydrodynamic (MHD) and Particle-in-Cell (PIC) Interlocked Simulation Model&quot;, ICPP2008: International Congress on Plasma Physics, Fukuoka, Japan (Sep. 8-12, 2008).</li></p>

<p><li>K. Kusano, &quot;The Three-Dimensional Dynamics of Solar Flare Onset Triggered by Flux Emerging&quot;, 37th COSPAR Scientific Assembly, Montreal, Canada (July 13-20, 2008).</li></p>

<p><li>K. Kusano, T. Sugiyama, S. Inoue, D. Shiota, E. Asano, T. Matsumoto, R. Kataoka, and K. Shibata, &quot;Multi-scale Interlocked Simulation of Solar Eruption&quot;, 37th COSPAR Scientific Assembly, Montreal, Canada (July 13-20, 2008).</li></p>

<p><li>S. Inoue, T. Magara, K. Takahashi, and T. Miyagoshi, &quot;Numerical Reconstruction of Sigmoidal Structure Associated with Flux Emergence on the Sun&quot;, Asia Oceania Geoscience Society 5th annual meeting, Busan, Korea (June 16-20, 2008).</li></p>

<p><br />
<div style="text-align: right;"><a href="#pagetop">&#8593;&nbsp;Page top</a>&nbsp;&nbsp;&nbsp;</div></p>

<p><br />
<li>K. Kusano, &quot;Can the 3D Magnetic Reconnection Account for Why Solar Flares Commence Suddenly?&quot;, Asia Oceania Geoscience Society 5th annual meeting, Busan, Korea (June 16-20, 2008).</li></p>

<p><li>K. Kusano, S. Inoue, D. Shiota, E. Asano, T. Matsumato, R. Kataoka, and K. Shibata, &quot;Data-driven Simulation of Solar Flare and CME Initiation&quot;, Asia Oceania Geoscience Society 5th annual meeting, Busan, Korea (June 16-20, 2008).</li></p>

<p><li>D. Shiota, K. Kusano, T. Miyoshi, K. Shibata, and N. Ohno, &quot;Launching Process of Coronal Mass Ejections and its Observability&quot;, Asia Oceania Geoscience Society 5th annual meeting, Busan, Korea (June 16-20, 2008).</li></p>

<p><li>T. Matsumoto, K. Shibata, E. Asano, K. Kusano, D. Shiota, S. Inoue, and R. Kataoka, &quot;Three-Dimensional Magnetohydrodynamic Simulation of Global Solar Corona for Space Weather Forecast&quot;, Astronum 2008, St John, USA (June 8-13, 2008).</li></p>

<p><li>K. Kusano, H. Hasegawa, S. Hirose, Y. Kawamura, A. Kawano, S. Shima, T. Sugiyama, D. Shiota, S. Inoue, R. Kataoka, E. Asano, T. Matsumato, T. Miyoshi. T. Ogino, T. Sugiyama, and K. Shibata, &quot;Study of Multi-scale and Multi-physics Dynamics with Macro-Micro Interlocked Simulations&quot;, The 6th EU-Japan Joint Symposium on Plasma Processing (JSPP2008) (Apr. 21-23, 2008).</li></p>

<p><br />
<div style="text-align: right;"><a href="#pagetop">&#8593;&nbsp;Page top</a>&nbsp;&nbsp;&nbsp;</div></p>

<p><br />
<li>R. Kataoka, D. Shiota, K. Kusano, T. Ogino, E. Asano, and K. Shibata, &quot;Interlocked MHD modeling of the initiation and propagation of coronal mass ejections in the inner heliosphere&quot;, 7th Annual International Astrophysics Conference, Particle acceleration and transport in the Heliosphere and Beyond, Kauai, Hawaii, USA (Mar. 7-13, 2008).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;Fluid-Particle Interlocked Simulations, -Basic Algorithm and Plasma Applications-&quot;, The US-Japan Workshop on Magnetic Reconnection 2008, Okinawa, (Mar. 5, 2008).</li></p>

<p><li>K. Kusano, D. Shiota, S. Inoue, R. Kataoka, E. Asano, T. Matsumato, T. Miyoshi, T. Ogino, T. Sugiyama, and K. Shibata, &quot;Study on the Trigger Mechanism of Solar Flares and Coronal Mass Ejections Based on Data-driven Simulations&quot;, The US-Japan Workshop on Magnetic Reconnection 2008, Okinawa, Japan (Mar. 3-6, 2008).</li></p>

<p><li>Shin-ichiro Shima, Kanya Kusano, Fumiaki Araki, Shintaro Kawahara, &quot;Super-Droplet Method for the Numerical Simulation of Clouds and Precipitation: a Particle-Based Microphysics Model Coupled with Non-hydrostatic Model&quot;, RIMS workshop on Fast Algorithms in Computational Fluids: theory and applications, RIMS, Kyoto Univ., Japan, (Feb. 20, 2008).</li></p>

<p><li>K. Kusano, D. Shiota, S. Inoue, R. Kataoka, E. Asano, T. Ogino, and K. Shibata, &quot;The Data-driven Simulation of Solar Flare and Coronal Mass Ejections&quot;, EARTH-SUN SYSTEM EXPLORATION ENERGY COUPLING WITHIN AND BETWEEN PLASMA REGIMES, Kona, Hawaii, USA (Jan. 14, 2008).</li><br />
</ul></p>

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<p><br />
<strong>2007</strong><ul><br />
<li>T. Sugiyama and K. Kusano, &quot;MHD-PIC interlocked simulation model in space plasma: application to collisionless shocks&quot;, American Geophysical Union (AGU) Fall Meeting 2007, San Francisco, USA (Dec. 13, 2007).</li><br />
<li>Shin-ichiro Shima, Kanya Kusano, Fumiaki Araki, Shintaro Kawahara, &quot;Towards the Evaluation of Cloud-Aerosol Interactions using Super-Droplet Method&quot;, 2007 AGU Fall Meeting, San Francisco, USA, (Dec. 10, 2007).</li><br />
<li>T. Sugiyama and K. Kusano, &quot;MHD-PIC interlocked simulation model in space plasma: application to collisionless shocks&quot;, International CAWSES Symposium, Kyoto, Japan (Oct. 26, 2007).</li></p>

<p><li>K. Kusano, H. Hasegawa, S. Hirose, Y. Kawamura, A. Kawano, S. Shima, and T. Sugiyama &quot;Competition and Synergy of Macro- and Micro-scale Physics Status and Prospects of Macro-Micro Interlocked Simulation&quot;, Joint Conference of 17th International Toki Conference on Physics of Flows and Turbulence in Plasmas and 16th International Stellarator/Heliotron Workshop 2007 (Plenary Talk) Toki, Japan (Oct. 15-19, 2007).</li></p>

<p><li>Shin-ichiro Shima and Kanya Kusano, &quot;A new attempt to understand the cosmic raycloud connection with super-droplet cloud microphysics model&quot;, EASTEC symposium 2007, Tohoku University, Japan, (Sep. 20, 2007).</li><br />
<li>A. Kawano and K. Kusano, &quot;Continuum/Particle Interlocked Simulation of Gas Detonation&quot;, 26th International Symposium on Shock Waves, G&#246;ttingen, Germany (July 15-20, 2007).</li></p>

<p><li>Shin-ichiro Shima, Kanya Kusano, Fumiaki Araki, and Shintaro Kawahara, &quot;Towards the Evaluation of Cloud-Aerosol Interactions using Super-Droplet Method&quot;, IUGG XXIV General Assembly, Perugia, Italy, (Jul. 2, 2007).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;MHD-PIC interlocked simulation model in space plasma: application to collisionless shocks&quot;, 2nd International Conference on Numerical Modeling of Space Plasma Flows ASTRONUM-2007, Paris, France (June 15, 2007).</li></p>

<p><li>I. Shinohara, Y. Kasaba, M. Fujimoto, M. Oka, S. Matsukiyo, Y. Seki, N. Shimada, T. Sugiyama, K. Tsubouchi, &quot;An expectation for the Cross-Scale/SCOPE missions: Collisionless shocks&quot;, European Geosciences Union General Assembly 2007, Vienna, Austria (Apr. 19, 2007).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;MHD-PIC Interlocked Simulation Model for Magnetic Reconnection&quot;, ISSS-8, Hawaii, USA (Feb. 25-Mar. 3, 2007).</li><br />
</ul></p>

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<p><strong>2006</strong><ul><li>T. Sugiyama, and K. Kusano, &quot;MHD-PIC Interlocked Simulation Model for Magnetic Reconnection&quot;, AGU Fall Meeting, San Francisco, USA (Dec. 14, 2006).</li></p>

<p><li>Shin-ichiro Shima, Shintaro Kawahara, Fumiaki Araki, Tooru Sugiyama, Akio Kawano, Shigenobu Hirose, and Kanya Kusano, &quot;Super-Droplet Method: a Particle-Based Cloud Microphysics Coupled with Nonhydrostatic Model&quot;, 2006 AGU Fall Meeting, San Francisco, USA 2006 (Dec. 11, 2006).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;MHD-PIC Interlocked Simulation Model for Magnetic Reconnection&quot;, CAWSES International Workshop on Space Weather Modeling, Yokohama, Japan (Nov. 17, 2006).</li></p>

<p><li>Shin-ichiro Shima, Shintaro Kawahara, Fumiaki Araki, Tooru Sugiyama, Akio Kawano, Shigenobu Hirose, and Kanya Kusano, &quot;Super-Droplet Method: a Particle-Based Cloud Microphysics Coupled with Nonhydrostatic Model&quot;, CAWSES International Workshop on Space Weather Modeling, Yokohama, Japan (Nov. 16, 2006).</li><br />
<li>A. Kawano and K. Kusano, &quot;Macro-micro Interlocked Simulation of Gas Detonation&quot;, CAWSES International Workshop on Space Weather Modeling, Yokohama, Japan (Nov. 14-17, 2006).</li></p>

<p><li>Shin-ichiro Shima, Shintaro Kawahara, Fumiaki Araki, Tooru Sugiyama, Akio Kawano, Shigenobu Hirose, and Kanya Kusano, &quot;Super-Droplet Method: a Novel Numerical Model of Clouds and Precipitation&quot;, The international workshop on high resolution &amp; cloud modeling, Kusatsu, Gumma, Japan (Oct. 3-5, 2006).</li></p>

<p><li>T. Sugiyama and K. Kusano, &quot;A new cross-scale simulation model connecting of MHD and PIC methods&quot;, Asia Oceania Geoscience Society 3rd Meeting, invited, Singapore (July 10, 2006).</li></ul></p>

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<p><strong>2005</strong><ul><li>K. Kusano, T. Maeshiro, T. Yokoyama, and T. Sakurai, &quot;Feedback Excitation of Double Reconnection as a Mechanism of the Impulsive Onset of Solar Flares&quot;, AGU Fall Meeting 2005, San Francisco, USA (Dec. 5-9, 2005).</li></p>

<p><li>T. Miyoshi and K. Kusano, &quot;An MHD Simulation of the Magnetosphere Based on the HLLD Approximate Riemann Solver&quot;, AGU Fall Meeting 2005, San Francisco, USA (Dec. 5-9, 2005).</li></p>

<p><li>T. Sugiyama, K. Kusano, A. Kageyama, S. Hirose, K. Watanabe, and T. Sato, &quot;MHD-PIC Connection Model of Auroral Arc Formation Process in a Magnetosphere-Ionosphere Coupling System&quot;, AGU Fall Meeting 2005, San Francisco, USA (Dec. 5-9, 2005).</li></p>

<p><li>Hirose, S., &quot;Local Dissipation and Radiative Transfer in Accretion Disks&quot;, Workshop on Magnetohydrodynamical Processes in Galaxies, Accretion Disks and in Star Forming Regions, Chiba, Japan, (Nov. 17-18, 2005).</li></p>

<p><li>K. Kusano, S. Inoue, D. Shiota, T. Yamamoto, Y. Miyoshi, T. Yokoyama, and T. Sakurai, &quot;Three-Dimensional Numerical Modeling of the Transition Process from Pre-Flare to Flare&quot;, STEREO/Solar-B Science Meeting, Hawaii, USA (Nov. 14-18, 2005).</li></p>

<p><br />
<div style="text-align: right;"><a href="#pagetop">&#8593;&nbsp;Page top</a>&nbsp;&nbsp;&nbsp;</div></p>

<p><br />
<li>S. Inoue, and K. Kusano, &quot;Simulation Study of Three-Dimensional and Nonlinear Dynamics of Flux Rope in the Solar Corona&quot;, 6th SOLAR-B Science Meeting, Kyoto, Japan (Nov. 8-11, 2005).</li></p>

<p><li>K. Kusano, S. Inoue, D. Shiota, T. Yamamoto, T. Yokoyama, and T. Sakurai, &quot;A Holistic Modeling of the Transition Process from Pre-Flare Sigmoid to Flare Eruption&quot;, 6th SOLAR-B Science Meeting, Kyoto, Japan (Nov. 8-11, 2005).</li></p>

<p><li>T. Yamamoto, K. Kusano, T. Yokoyama, and T. Sakurai, &quot;Helicity Injections in Regions of Various Magnetic Fluxes&quot;, 6th SOLAR-B Science Meeting, Kyoto, Japan (Nov. 8-11, 2005).</li></p>

<p><li>K. Kusano, &quot;Interlocking models for multi-scale simulations&quot;. JIFT Workshop, Kasuga, Fukuoka, Japan (Sep. 13, 2005).</li></p>

<p><li>Hiroki Hasegawa, Seiji Ishiguro, and Masao Okamoto, &quot;Distributed Parallelization of Exact Charge Conservative Particle Simulation Code by High-Performance Fortran&quot;, HPF International Workshop: Experiences and Progress (part of the 6th International Symposium on High Performance Computing), Nara, Japan (Sep. 7, 2005).</li></p>

<p><br />
<div style="text-align: right;"><a href="#pagetop">&#8593;&nbsp;Page top</a>&nbsp;&nbsp;&nbsp;</div></p>

<p><br />
<li>K. Kusano, S. Inoue, T. Sakurai, and T. Yokoyama, &quot;Simulation Study on the Self-Organization of Sigmoidal Structure and the Onset of Solar Flares&quot;, International scientific conference &quot;Chromospheric and Coronal Magnetic Fields&quot;, Katlenburg-Lindau, Germany (Aug. 30-Sep. 2, 2005).</li></p>

<p><li>T. Sugiyama and M. Fujimoto, &quot;Particle interactions with wavy/turbulent structure at high Mach number shock surface&quot; IAGA 2005 Scientific Assembly, Toulouse, France (July 26, 2005).</li></p>

<p><li>Hiroki Hasegawa, Seiji Ishiguro, and Masao Okamoto, &quot;Particle Acceleration by a Large Amplitude Wave Associated with an Ion Beam in a Magnetized Plasma&quot;, Joint conference of 19th International Conference on Numerical Simulation of Plasmas and 7th Asia Pacific Plasma Theory Conference, Nara, Japan (July 12-15, 2005).</li></p>

<p><li>Seiji Ishiguro and Hiroki Hasegawa, &quot;Three-Dimensional Particle-In-Cell Simulation of Scrape-off-Layer Plasmas&quot;, Joint conference of 19th International Conference on Numerical Simulation of Plasmas and 7th Asia Pacific Plasma Theory Conference, Nara, Japan (July 12-15, 2005).</li></p>

<p><li>K. Kusano, N. Nishikawa, S. Inoue, T. Maeshiro, and T. Sakurai, &quot;Simulation Study of the Solar Flare Onset Mechanism and the Self-Organization in the Solar Coronal Plasma&quot;, The joint conference of 19th International Conference on Numerical Simulation of Plasmas and Asia Pacific Plasma Theory Conference, Nara, Japan (July 12-15, 2005).</li></p>

<p><br />
<div style="text-align: right;"><a href="#pagetop">&#8593;&nbsp;Page top</a>&nbsp;&nbsp;&nbsp;</div></p>

<p><br />
<li>N. Ohno, A. Kageyama, and K. Kusano, &quot;Virtual Reality Visualization by CAVE with VFIVE and VTK&quot;, The joint conference of 19th International Conference on Numerical Simulation of Plasmas and Asia Pacific Plasma Theory Conference, Nara, Japan (July 12-15, 2005).</li></p>

<p><li>Yukiharu Ohsawa, Ken Kato, and Hiroki Hasegawa, &quot;Simulation Studies of Positron Acceleration by a Shock Wave&quot;, Joint conference of 19th International Conference on Numerical Simulation of Plasmas and 7th Asia Pacific Plasma Theory Conference, Nara, Japan (July 12-15, 2005).</li></p>

<p><li>T. Sugiyama, K. Kusano, S. Hirose, and K. Kageyama, &quot;MHD-PIC Connection Model in a Magnetosphere-Ionosphere Coupling System&quot;, The joint conference of 19th International Conference on Numerical Simulation of Plasmas and Asia Pacific Plasma Theory Conference, Nara, Japan (July 12-15, 2005).</li></p>

<p><li>S. Shima and Y. Kuramoto, &quot;Rotating Spiral Waves with Phase-Randomized Core in Nonlocally Coupled Oscillators&quot;, SIAM conference on applications of dynamical systems, Snowbird, USA (May 22-26, 2005).</li></p>

<p><li>K.Kusano, &quot;Magnetic Relaxation in the Solar Corona&quot;, The Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas (CMSO) topical meeting, Princeton, USA (Apr. 27-30, 2005).</li></p>

<p><li>K. Kusano, &quot;Numerical Modeling of Active Regions and Solar Flares&quot; 2005 International Workshop on Space Weather - On the Causes of Southward Interplanetary Magnetic Field (IMF), Tokyo, Japan (Apr. 4-6, 2005).</li><br />
</ul></p>

<p><br />
<div style="text-align: right;"><a href="#pagetop">&#8593;&nbsp;Page top</a>&nbsp;&nbsp;&nbsp;</div></p>

<p><br />
<table border="0" cellspacing="2" cellpadding="4" bgcolor="#e7f4f4" width="100%"><tr><td valign="top"><strong>Books</strong></td></tr></table></p>

<ul><li>Sakaguchi, H., Kusano, K., and Suetsugu D., eds., &quot;Multi-Structure Dynamics -- Universal Law in the Life, Space and Earth Science&quot;,University of Tokyo Press (2008) (Japanese).</li>
]]>
        
    </content>
</entry>

<entry>
    <title>Links</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/links/links.html" />
    <id>tag:hsrp.jamstec.go.jp,2009:/hsrp/en//3.38</id>

    <published>2009-01-27T04:55:53Z</published>
    <updated>2009-03-06T07:44:02Z</updated>

    <summary>Government OfficesMinistry of Education,culture,sports,science and technology-japan (MEXT) Universities and Research Organizations Japan Agency for Marine-Earth Science and Technology (JAMSTEC) ・The E...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Links" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<p><strong>Government Offices</strong><ul><li><a href="http://www.mext.go.jp/english/" target="_blank">Ministry of Education,culture,sports,science and technology-japan (MEXT)</a></li><br />
</ul></p>

<p><br />
<strong>Universities and Research Organizations</strong><ul><br />
<li><a href="http://www.jamstec.go.jp/e/" target="_blank">Japan Agency for Marine-Earth Science and Technology (JAMSTEC)</a><br />
<div style="margin:10px 0px 0px 15px ">・<a href="http://www.jamstec.go.jp/esc/index.en.html" target="_blank">The Earth Simulator Center (ESC)</a><br />
・<a href="http://www.jamstec.go.jp/ifree/eng/index.html" target="_blank">Institute For Research on Earth Evolution (IFREE)</a></div><br />
</li><br />
<li><a href="http://www.titech.ac.jp/home.html" target="_blank">Tokyo Institute of Technology </a><br />
<div style="margin:10px 0px 0px 15px ">・<a href="http://www.sci.titech.ac.jp/english/index.html" target="_blank">Graduate School of Science</a></div><div style="margin:5px 0px 0px 35px ">&#9507;&nbsp;<a href="http://www.ircs.titech.ac.jp/index.html" target="_blank">Interactive Research Center of Science</a><br />
&#9495;&nbsp;<a href="http://www.geo.titech.ac.jp/english_index.php" target="_blank">Department of Earth and Planetary Sciences</a></div><br />
</li><br />
<li><a href="http://www.stelab.nagoya-u.ac.jp/ste-www1/index.html" target="_blank">Nagoya University</a><div style="margin:10px 0px 0px 15px ">・<a href="http://www.stelab.nagoya-u.ac.jp/ste-www1/index.html" target="_blank">Solar-Terrestrial Environment Laboratory (STEL)</a><br />
</div></li><br />
<li><a href="http://www.hiroshima-u.ac.jp/" target="_blank">Hiroshima University</a>　<br />
<div style="margin:10px 0px 0px 15px ">・<a href="http://www.hiroshima-u.ac.jp/en/adsm/" target="_blank">Graduate School of Advanced Sciences of Matter (AdSM)</a><br />
・<a href="http://www.hiroshima-u.ac.jp/sci/" target="_blank">Graduate School of Science</a></div><div style="margin:5px 0px 0px 35px ">&#9495;&nbsp;<a href="http://insam.sci.hiroshima-u.ac.jp/" target="_blank">Institute for Nonlinear Scinences and Applied Mathematics(iINSAM)</a></div></li><br />
<li><a href="http://www.meiji.ac.jp/cip/english/" target="_blank">Meiji University</a><br />
<div style="margin:10px 0px 0px 15px ">・<a href="http://www.meiji.ac.jp/cip/english/graduate_education/science.html" target="_blank">Department of Science and Technology</a><br />
・<a href="http://www.mims.meiji.ac.jp/index-e.html" target="_blank">Meiji Institute for Advanced Study of Mathematical Sciences (MIMS)</a></div></li><br />
<li><a href="/jswm/en/" target="_blank">Joint Project for Space Weather Modeling </a></li><br />
</ul></p>

<p><br />
<strong>Academic Societies</strong><ul><li><a href="http://www.sgepss.org/sgepss/index-e.html" target="_blank">Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS)</a></li></p>

<p><li><a href="http://wwwsoc.nii.ac.jp/msj/index-e.html" target="_blank">Meteorological Society of Japan (MSJ)</a></li></p>

<p><li><a href="http://www.sccj.net/e/index.htm" target="_blank">Journal of Computer Chemistry, Japan (SCCJ)</a></li></p>

<p><li><a href="http://www.asj.or.jp/index.html.en" target="_blank">The Astronomical Society of Japan (ASJ)</a></li></p>

<p><li><a href="http://wwwsoc.nii.ac.jp/jps/english/index.html" target="_blank">The Physical Society of Japan (PSJ)</a></li></p>

<p><li><a href="http://www.jspf.or.jp/index.html.en" target="_blank">The Japan Society of Plasma Science and Nuclear Fusion Research (JSPF)</a></li></p>

<p><li><a href="http://www.mol-sim.jp/" target="_blank">Molecular Simulation Society of Japan (MSSJ)</a></li></p>

<p><li><a href="http://www.aas.org/" target="_blank">American Astronomical Society (AAS)</a></li></p>

<p><li><a href="http://www.agu.org/" target="_blank">American Geophysical Union (AGU)</a></li></p>

<p><li><a href="http://www.aps.org/" target="_blank">American Physical Society (APS)</a></li></p>

<p><li><a href="http://www.iau.org/" target="_blank">International Astronomical Union (IAU)</a></li></p>

<p><li><a href="http://www.siam.org/" target="_blank">Society for Industrial and Applied Mathematics (SIAM)</a></li><br />
</ul> </p>]]>
        
    </content>
</entry>

<entry>
    <title>International Workshop on Variabilities of Solar-Cosmic and Terrestrial Environment, Yokohama (Dec. 4-6, 2008)</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/events/event081204.html" />
    <id>tag:hsrp.jamstec.go.jp,2008:/hsrp/en//3.117</id>

    <published>2008-12-04T06:03:39Z</published>
    <updated>2009-03-18T04:16:30Z</updated>

    <summary> Workshop site:  http://www.ircs.titech.ac.jp/workshop/...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Events" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<span class="mt-enclosure mt-enclosure-image" style="display: inline;"><img alt="event08title.jpg" src="/hsrp/en/images/event08title.jpg" width="510" height="721" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 20px;" /></span><p>
Workshop site: 
<a href="http://www.ircs.titech.ac.jp/workshop/">http://www.ircs.titech.ac.jp/workshop/</a></p>]]>
        
    </content>
</entry>

<entry>
    <title>Workshop on &quot;Multi-Structure Dynamics + Mathematical Sciences Based on Modeling and Analysis&quot;, Atami (Nov. 30 - Dec. 1, 2008)</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/events/event081130.html" />
    <id>tag:dagashiya.yes.jamstec.go.jp,2008:/hsrp/en//3.116</id>

    <published>2008-09-20T06:02:32Z</published>
    <updated>2009-03-12T04:39:04Z</updated>

    <summary> ...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Events" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<span class="mt-enclosure mt-enclosure-image" style="display: inline;"><img alt="swa08a1.jpg" src="/hsrp/en/swa08a1.jpg" class="mt-image-none" style="" width="510" height="341" /></span>
<br><br>
<span class="mt-enclosure mt-enclosure-image" style="display: inline;"><img alt="swa08a2.jpg" src="/hsrp/en/images/swa08a2.jpg" width="510" height="327" class="mt-image-none" style="" /></span>
<br><br>
<span class="mt-enclosure mt-enclosure-image" style="display: inline;"><img alt="swa08a3.jpg" src="/hsrp/en/images/swa08a3.jpg" width="512" height="230" class="mt-image-none" style="" /></span>
<br><br>
<span class="mt-enclosure mt-enclosure-image" style="display: inline;"><a href="/hsrp/en/assets_c/2009/03/swa08a4-306.html" onclick="window.open('/hsrp/en/assets_c/2009/03/swa08a4-306.html','popup','width=1024,height=504,scrollbars=no,resizable=no,toolbar=no,directories=no,location=no,menubar=no,status=no,left=0,top=0'); return false"><img src="/hsrp/en/assets_c/2009/03/swa08a4-thumb-510x251-306.jpg" width="510" height="251" alt="swa08a4.jpg" class="mt-image-none" style="" /></a></span>
]]>
        
    </content>
</entry>

<entry>
    <title>JAMSTEC Workshop on &quot;Multi-Structure Dynamics&quot;, Yugawara (Mar. 28-29, 2008)</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/events/event08328.html" />
    <id>tag:dagashiya.yes.jamstec.go.jp,2008:/hsrp/en//3.115</id>

    <published>2008-04-01T05:59:45Z</published>
    <updated>2009-03-12T04:39:13Z</updated>

    <summary> ...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Events" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
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    </content>
</entry>

<entry>
    <title>Cloud Formation</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/research/cloud-formation.html" />
    <id>tag:hsrptest.yes.jamstec.go.jp,2008:/hsrp/en//3.91</id>

    <published>2008-01-07T13:36:03Z</published>
    <updated>2009-06-19T13:39:31Z</updated>

    <summary>Macro-Micro Interlocked Simulation of Cloud Formation We have developed a novel, particle based, probabilistic simulation model of cloud microphysics named the Super-Droplet Method (SDM). SDM enables ...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Research" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<p><strong>Macro-Micro Interlocked Simulation of Cloud Formation</strong></p>

<p>We have developed a novel, particle based, probabilistic simulation model of cloud microphysics named the Super-Droplet Method (SDM). SDM enables accurate simulation of cloud microphysics, such as the condensation and evaporation of cloud particles, the coalescence of cloud particles, and the sedimentation of precipitation particles with less demanding cost in computation. The new model could be useful for weather forecasts, the optimization of artificial rain, and improving the scientific understanding of climate change. <br />
<a name="zu01"></a></p>

<p><a href="/hsrp/ja/movies/cloud.html" target="_balnk"  title="Cloud formation and rainfall simulation"><img src="/hsrp/ja/assets_c/2009/02/cloud1-thumb-450x252-69.gif" width="450" height="252" alt="cloud1.gif" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 20px;" /></a><small><strong>[&#8593; click the figure to see the movie ]</strong></small><br />
<small>Maritime cumulus formation and rainfall simulated by the coupled model of SDM and non-hydrostatic model. <br />
</small><br />
<a name="zu02"></a><br />
<img alt="simulation model" src="/hsrp/ja/images/research/cloud2.gif" width="525" height="385" class="mt-image-none" style="" /></p>

<p><small>It is one of our enterprising research subjects to develop a multi-scale simulation model that consists of a global atmospheric simulation and a regional scale simulation. The figure is a schematic overview of the coupled simulation in which seasonal rain fronts calculated by AFES (Atmosphere for Earth Simulator) is sampled for regional calculations. The Super-Droplet Method would be used in the regional model.</small><br />
</p>]]>
        
    </content>
</entry>

<entry>
    <title>Aerosols</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/research/aerosols.html" />
    <id>tag:210.251.87.117,2009:/hsrp/en//3.92</id>

    <published>2008-01-06T13:03:00Z</published>
    <updated>2009-03-12T04:41:57Z</updated>

    <summary>Molecular Simulation of Aerosol Nucleation It is an important research subject to quantitatively evaluate the production rate of atmospheric aerosols because atmospheric aerosols, which act as cloud c...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Research" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<p><strong>Molecular Simulation of Aerosol Nucleation</strong></p>

<p>It is an important research subject to quantitatively evaluate the production rate of atmospheric aerosols because atmospheric aerosols, which act as cloud condensation nuclei, significantly affect the Earth's climate. However, we cannot still directly observe the nucleation process of atmospheric aerosols occurring at the nanometer scale. The holistic simulation research program is trying to quantitatively understand the nucleation process of aerosols using a combination of ab initio quantum calculations and classical molecular dynamics simulations. </p>

<div style="text-align: center;"><span class="mt-enclosure mt-enclosure-image" style="display: inline;"><img alt="Nucleation process of sulfuric acid aerosols" src="/hsrp/ja/images/research/aerosol1.jpg" width="450" height="338" class="mt-image-none" style="" /></span></div>
<strong>
<small>Nucleation process of sulfuric acid aerosols.</small></strong>

<p><span class="mt-enclosure mt-enclosure-image" style="display: inline;"><img alt="Homogeneous vapor-liquid nucleation of water" src="/hsrp/ja/images/research/aerosol2.jpg" width="525" height="527" class="mt-image-none" style="" /></span><br />
<strong><small><br />
Homogeneous vapor-liquid nucleation of water.</small></strong></p>]]>
        
    </content>
</entry>

<entry>
    <title>Auroral Arc Formation</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/research/auroral-arc-formation.html" />
    <id>tag:210.251.87.117,2009:/hsrp/en//3.94</id>

    <published>2008-01-05T12:45:53Z</published>
    <updated>2009-03-12T04:43:48Z</updated>

    <summary>  Holistic Simulation of Auroral Arc Formation A holistic simulation of the aurora formation process has been developed by connecting a magnetohydrodynamic model with a microscopic particle model. The...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Research" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<p> <strong> Holistic Simulation of Auroral Arc Formation</strong></p>

<p>A holistic simulation of the aurora formation process has been developed by connecting a magnetohydrodynamic model with a microscopic particle model. The simulation can handle consistently both the macroscopic dynamics in the magnetospheric region and electron acceleration on the ionosphere-magnetosphere boundary.</p>

<p><img alt="Holistic Simulation of Auroral Arc Formation" src="/hsrp/ja/images/research/hargproj2b.jpg" width="450" height="338" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 20px;" /><center><table width="450" border="0" cellpadding="0" cellspacing="0"><tr><td><small>The solar wind interacts with the geomagnetic field resulting in the formation of the magnetosphere, which is roughly balanced between the solar wind pressure and the geomagnetic pressure whereby twin vortices are formed basically in the magnetospheric equatorial plane. </small></td></tr></table></center></p>

<p><img alt=" Holistic Simulation of Auroral Arc Formation" src="/hsrp/ja/images/research/hargproj2c.jpg" width="450" height="332" class="mt-image-center" style="text-align: center; display: block; margin: 0 auto 20px;" /></form><center><table width="450" border="0" cellpadding="0" cellspacing="0"><tr><td><small>Downward electrons are strongly energized to produce excitation of oxygen and nitrogen molecules at the ionosphere. The ionospheric density is also strongly modulated by the local enhancement of ionization, which in turn changes the evolution of the magnetosphere-ionosphere current system. </small></td></tr></table></center><br />
</p>]]>
        
    </content>
</entry>

<entry>
    <title>Space plasmas</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/research/space-plasmas.html" />
    <id>tag:210.251.87.117,2009:/hsrp/en//3.93</id>

    <published>2008-01-04T12:45:19Z</published>
    <updated>2009-03-12T04:43:39Z</updated>

    <summary>Macro-Micro Interlocked Simulation of Explosive Plasma Phenomena in Space and the Solar Corona Explosive energy liberation, known as solar flares, occurs in the solar corona filled with high-temperatu...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Research" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[<p><strong>Macro-Micro Interlocked Simulation of Explosive Plasma Phenomena in Space and the Solar Corona</strong></p>

<p>Explosive energy liberation, known as solar flares, occurs in the solar corona filled with high-temperature plasma. Shock waves and high-energy particles emitted from the explosion may damage long distant power transmission systems and spacecraft around the Earth and, sometimes, endanger astronauts in space. In order to forecast solar flares and the effect on the Earth, we are developing interlocked plasma simulations to reveal both large-scale plasma dynamics and small-scale plasma kinetics in the flaring region as well as in the inside of shocks.</p>

<p><img alt="Plasma simulation" src="/hsrp/ja/assets_c/2009/02/plasma1-thumb-525x245-75.jpg" width="525" height="245" class="mt-image-none" style="" /></p>

<p><small>(Left) magnetic field model of the solar corona, (middle) magnetohydrodynamic simulation of ejective solar flare and (right) particle-in-cell simulation of magnetic reconnection, which causes solar flare explosions.</small></p>

<p><img alt="Plasma simulation" src="/hsrp/ja/images/research/plasma2.jpg" width="500" height="489" class="mt-image-none" style="" /></p>

<p><small>High-resolution micro-scale simulation of a shock wave in plasma: It shows that waves are emitted from the shock wave front into the upstream region. Such waves are useful as precursors of shock wave attacks</small></p>]]>
        
    </content>
</entry>

<entry>
    <title>JAMSTEC banner</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/banner/jamstec-banner.html" />
    <id>tag:210.251.87.117,2009:/hsrp/en//3.108</id>

    <published>2007-01-10T14:52:27Z</published>
    <updated>2009-03-18T04:42:51Z</updated>

    <summary></summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="banner" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
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        http://www.jamstec.go.jp/e/
    </content>
</entry>

<entry>
    <title>IFREE banner</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/banner/ifree-banner.html" />
    <id>tag:hsrp.jamstec.go.jp,2009:/hsrp/en//3.138</id>

    <published>2007-01-08T07:23:24Z</published>
    <updated>2009-03-12T04:43:06Z</updated>

    <summary> ...</summary>
    <author>
        <name>esc</name>
        
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        <category term="banner" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
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        http://www.jamstec.go.jp/ifree/eng/index.html
    </content>
</entry>

<entry>
    <title>ESC Banner</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/banner/esc-banner.html" />
    <id>tag:hsrp.jamstec.go.jp,2009:/hsrp/en//3.137</id>

    <published>2007-01-07T07:21:05Z</published>
    <updated>2009-05-19T08:32:23Z</updated>

    <summary> ...</summary>
    <author>
        <name>esc</name>
        
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        <category term="banner" scheme="http://www.sixapart.com/ns/types#category" />
    
    
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        http://www.jamstec.go.jp/esc/
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</entry>

<entry>
    <title>JSWM　banner</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/banner/jswmbanner.html" />
    <id>tag:hsrp.jamstec.go.jp,2009:/hsrp/en//3.113</id>

    <published>2007-01-05T04:04:12Z</published>
    <updated>2009-03-12T04:43:16Z</updated>

    <summary> ...</summary>
    <author>
        <name>esc</name>
        
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        <category term="banner" scheme="http://www.sixapart.com/ns/types#category" />
    
    
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        /jswm/en/
    </content>
</entry>

<entry>
    <title>CAWSES International Workshop on Space Weather Modeling (CSWM), Yokohama(Nov. 14-17, 2006)</title>
    <link rel="alternate" type="text/html" href="http://www.jamstec.go.jp/less/space_earth/en/events/event061114.html" />
    <id>tag:dagashiya.yes.jamstec.go.jp,2006:/hsrp/en//3.34</id>

    <published>2006-10-01T04:52:03Z</published>
    <updated>2009-03-12T04:40:36Z</updated>

    <summary> Advancement in our understanding of the space environment is in great demand now as the dynamic activities of the Sun, solar wind, magnetosphere and ionosphere can influence modern technology systems...</summary>
    <author>
        <name>esc</name>
        
    </author>
    
        <category term="Events" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="ja" xml:base="http://www.jamstec.go.jp/less/space_earth/en/">
        <![CDATA[
Advancement in our
understanding of the space environment is in great demand now as the
dynamic activities of the Sun, solar wind, magnetosphere and ionosphere
can influence modern technology systems and endanger human life and
health. The numerical simulation and modeling driven by integrated
observations are powerful methods for understanding the complex
Sun-Earth system, and they are an important means for predicting space
weather. To address this issue, a workshop on <strong>"CAWSES International Workshop on Space Weather Modeling (CSWM)"</strong> will be held at <a href="http://web.archive.org/web/20061213224716/http://www.es.jamstec.go.jp/">the Earth Simulator Center</a>
in Yokohama, Japan. This workshop will provide a forum for review of
the recent progress and the scientific challenges in space weather
modeling research.

<h2>Workshop Venue & Host Institute</h2>
<blockquote>The Earth Simulator Center, <br>
Japan Agency for Marine-Earth Science and Technology 
(JAMSTEC) <br>
3173-25 Showa-machi, Kanazawa-ku, Yokohama 236-0001, Japan.</blockquote>

<h2>Scientific Organizing Committee</h2>
<ul>
	<li>K. Shibata (Co-chair, Kyoto University, Japan)</li>
	<li>K. Kusano (Co-chair, The Earth Simulator Center, Japan)</li>
	<li>J. Buechner (Max-Planck.Institut fuer Sonnensystemforschung, Germany)</li>
	<li>T. I. Gombosi (The University of Michigan, USA)</li>
	<li>N. Gopalswamy (NASA, Goddard Space Flight Center, USA)</li>
	<li>N. Gopalswamy (NASA, Goddard Space Flight Center, USA)</li>
	<li>M. Hesse (NASA, Goddard Space Flight Center, USA)</li>
	<li>J. U. Kozyra (The University of Michigan, USA)</li>
	<li>J. Lin (Yunnan Astronomical Observatory, China; Harvard-Smithsonian Center for Astrophysics, USA)</li>
	<li>T. Ogino (Nagoya University, Japan)</li>
	<li>B. Sanahuja (Universitat de Barcelona, Spain)</li>
	<li>S. T. Wu (University of Alabama in Huntsville, USA)</li>
</ul>

<h2>Local Organizing Committee</h2>
<ul>
	<li>M. Fujimoto (JAXA/ISAS)</li>
	<li>S. Hirose (ESC/JAMSTEC)</li>
	<li>M. Hoshino (U. Tokyo)</li>
	<li>K. Kusano (ESC/JAMSTEC)</li>
	<li>T. Miyoshi (Hiroshima U.)</li>
	<li>T. Obara (NiCT)</li>
	<li>M. Oka (Kyoto U.)</li>
	<li>Y. Omura (Kyoto U.)</li>
	<li>T. Sakurai (NAOJ)</li>
	<li>K. Shibata (Kyoto U.)</li>
	<li>T. Sugiyama (ESC/JAMSTEC)</li>
	<li>S. Tsuneta (NAOJ)</li>
	<li>M. Ugai (Ehime U.)</li>
	<li>T. Yokoyama (U. Tokyo)</li>
</ul>

<h2>Co-Sponsorship</h2>
<ul>
	<li>Grant-in-Aid of the MEXT of Japan for Creative Scientific Research "The Basic Study of Space Weather Prediction"</li>
	<li>CAWSES/SCOSTEP</li>
	<li>Solar-Terrestrial Environment Laboratory, Nagoya University</li>
	<li>Research Institute for Sustainable Humanosphere (RISH), Kyoto University</li>
</ul>

<h2>Program</h2>
<blockquote><f<span class="mt-enclosure mt-enclosure-file" style="display: inline;"><a href="/hsrp/en/pdf/Contents_WEB.pdf">Program (PDF : 113KB) </a></span></blockquote>

<h2>Abstracts</h2>
<blockquote><span class="mt-enclosure mt-enclosure-file" style="display: inline;"><a href="/hsrp/en/pdf/Abstracts.pdf">Abstracts (PDF : 6668KB)</a></span></blockquote>

<h2>Japanese Tea Ceremony</h2>
<blockquote><span class="mt-enclosure mt-enclosure-file" style="display: inline;"><a href="/hsrp/en/pdf/Tea.pdf">Ceremony (PDF : 1.22MB) </a></span></blockquote>



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