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NAKASHIMA RyosukeGraduate School of System Informatics / Department of System InformaticsAssistant Professor
Research activity information
■ Award- Nov. 2021 SGEPSS, SGEPSS Paper Award, A candidate secular variation model for IGRF-13 based on MHD dynamo simulation and 4DEnVar data assimilationJapan society
- Jul. 2016 Japan Geoscience Union, JpGU 2016 Outstading Student Presentation Award, The empirical mode analysis of the decadal variations in the geomagnetic Gauss coefficientsJapan society
- An hourglass is known to become slightly heavier while the sand is falling. We quantitatively reproduced this minute weight change through numerical simulation. By treating the hourglass as a mechanical system of coupled variable-mass objects, we find that two effects contribute equally to the weight variation: the linear change in the thickness of the sand layers and the progressive shortening of the free-fall distance of the sand grains. Based on this analysis, we developed a discrete element simulation using the soft-sphere approach. In this model, sand grains fall at a constant rate and accumulate into multiple vertical piles. The simulation, implemented in Processing, can be run on a standard notebook PC.Japan Society for Simulation Technology, 2026, Transaction of the Japan Society for Simulation Technology, 18(1) (1), 1 - 10, Japanese[Refereed]
- Elsevier BV, May 2025, Results in Applied Mathematics, 26, 100594[Refereed]Scientific journal
- Informa UK Limited, Aug. 2024, Geophysical & Astrophysical Fluid Dynamics, 118(5-6) (5-6), 387 - 440[Refereed]Scientific journal
- Abstract We have submitted a secular variation (SV) candidate model for the thirteenth generation of International Geomagnetic Reference Field model (IGRF-13) using a data assimilation scheme and a magnetohydrodynamic (MHD) dynamo simulation code. This is the first contribution to the IGRF community from research groups in Japan. A geomagnetic field model derived from magnetic observatory hourly means, and CHAMP and Swarm-A satellite data, has been used as input data to the assimilation scheme. We adopt an ensemble-based assimilation scheme, called four-dimensional ensemble-based variational method (4DEnVar), which linearizes outputs of MHD dynamo simulation with respect to the deviation from a dynamo state vector at an initial condition. The data vector for the assimilation consists of the poloidal scalar potential of the geomagnetic field at the core surface and flow velocity field slightly below the core surface. Dimensionless time of numerical geodynamo is adjusted to the actual time by comparison of secular variation time scales. For SV prediction, we first generate an ensemble of dynamo simulation results from a free dynamo run. We then assimilate the ensemble to the data with a 10-year assimilation window through iterations, and finally forecast future SV by the weighted sum of the future extension parts of the ensemble members. Hindcast of the method for the assimilation window from 2004.50 to 2014.25 confirms that the linear approximation holds for 10-year assimilation window with our iterative ensemble renewal method. We demonstrate that the forecast performance of our data assimilation and forecast scheme is comparable with that of IGRF-12 by comparing data misfits 4.5 years after the release epoch. For estimation of our IGRF-13SV candidate model, we set assimilation window from 2009.50 to 2019.50. We generate our final SV candidate model by linear fitting for the weighted sum of the ensemble MHD dynamo simulation members from 2019.50 to 2025.00. We derive errors of our SV candidate model by one standard deviation of SV histograms based on all the ensemble members.Springer Science and Business Media LLC, Sep. 2020, Earth, Planets and Space, 72(1) (1), English, International magazine, Co-authored internationally[Refereed]Scientific journal
- Aug. 2026, 第53回 可視化情報シンポジウム 講演論文集, Japanese
- Aug. 2026, 第53回 可視化情報シンポジウム 講演論文集, Japanese
- 東京 : 日本計算工学会, Jun. 2025, 計算工学講演会論文集 = Proceedings of the Conference on Computational Engineering and Science / 日本計算工学会 編, 30, 824 - 829, Japanese最小二乗SPH法の打切り誤差に基づく古典的SPH法の離散化誤差の検証—Verification of the discretization error of classical SPH models based on the truncation error of the least squares SPH method
- 東京 : 日本計算工学会, Jun. 2024, 計算工学講演会論文集 = Proceedings of the Conference on Computational Engineering and Science / 日本計算工学会 編, 29, 809 - 814, Japanese最小二乗法を用いたSPH法の高精度化について—A high-accuracy SPH method using the least-squares method
- Feb. 2020, Doctoral Thesis (Kyushu University), EnglishOthers
- 京都大学 大学院理学研究科 附属地磁気世界資料解析センター, Jan. 2019, 地磁気世界資料解析センター ニュース, (173) (173), JapaneseOthers
- 第53回 可視化情報シンポジウム, Aug. 2026, Japanese, Ishikawa, Japan, Domestic conferenceVisualization Analysis of Reversal-like Events in a Regular Tetrahedral MHD Dynamo ModelOral presentation
- 第53回 可視化情報シンポジウム, Aug. 2026, Japanese, Ishikawa, Japan, Domestic conferenceVisualization of 3D Fluid Simulations Using MirrorsOral presentation
- JpGU-AGU Joint Meeting 2026, May 2026, English, Chiba, Japan, International conferenceCan quasi-modes in a stratified layer at the top of the Earth's core be observed in geomagnetic fluctuations?Poster presentation
- JpGU-AGU Joint Meeting 2026, May 2026, English, Chiba, Japan, International conferenceReversal-like Events in a Regular Tetrahedral MHD Dynamo ModelPoster presentation
- 「⾒る可視化」から「調べる可視化」、「⾒せる可視化」へ 先進的可視化表現法とデータ科学の研究会 (VR2025), Dec. 2025, Japanese, 岐阜, Japan2次元可視化ライブラリ slice-svg 向けブラウザビューアの開発Oral presentation
- 「⾒る可視化」から「調べる可視化」、「⾒せる可視化」へ 先進的可視化表現法とデータ科学の研究会 (VR2025), Dec. 2025, Japanese, 岐阜, Japan傾斜⽴⽅体容器中の熱対流とその可視化Oral presentation
- 非線形プラズマ科学研究会 2025, Dec. 2025, Japanese, 福岡, Japan回転球面上の 2 次元非圧縮 MHD 波の quasi-modeOral presentation
- 第30回計算工学講演会, Jun. 2025, Japanese, Japan, Domestic conferenceVerification of the discretization error of classical SPH models based on the truncation error of the least squares SPH methodOral presentation
- Japan Geoscience Union Meeting 2025, May 2025, Japanese, Chiba, Japan, Domestic conferenceVerification of the Equation of the Flight Distance of a Sand Particle over Wind Ripples in the Nishimori Model by using Numerical AnalysisPoster presentation
- Japan Geoscience Union Meeting 2025, May 2025, Japanese, Chiba, Japan, Domestic conferenceLinear stability analysis of Boussinesq convection with explicit methods and its verification using a high-precision particle schemeOral presentation
- 地球流体セミナー 分科会, Mar. 2025, Japanese, 北海道 支笏湖, Japan木星内部安定成層の MAC 波Others
- 非線形プラズマ科学研究会 2024, Dec. 2024, Japanese, 福岡, Japan回転球面上の2次元非圧縮MHD波の波線理論的アプローチOral presentation
- 8th Asia-Pacific Conference on Plasma Physics, Nov. 2024, English, Malacca, Malaysia, International conferenceA ray-theoretical approach to investigate continuous spectra of two-dimensional incompressible MHD waves on a rotating sphere[Invited]Invited oral presentation
- 日本惑星科学会2024年秋季講演会, Sep. 2024, Japanese, Fukuoka, Japan, Domestic conferenceFormulation and implementation of the least squares SPH methodOral presentation
- 日本惑星科学会2024年秋季講演会, Sep. 2024, Japanese, Fukuoka, Japan, Domestic conferenceMagnetohydrodynamic waves in a stably stratified region of Jupiter’s interiorPoster presentation
- The 18th Symposium of SEDI (Study of the Earth’s Deep Interior), Jun. 2024, English, Great Barrington, MA, United States, International conferenceA ray-theoretical approach to investigate two-dimensional MHD waves in a stably stratified layerPoster presentation
- 第29回計算工学講演会, Jun. 2024, Japanese, 神戸, Japan, Domestic conference最小二乗法を用いたSPH法の高精度化についてOral presentation
- Japan Geoscience Union Meeting 2024, May 2024, Japanese, Chiba, Japan, Domestic conferenceHigh accuracy particle method for simulating planetary interiors and its numerical stability analysisOral presentation
- Japan Geoscience Union Meeting 2024, May 2024, Japanese, Chiba, Japan, Domestic conferencequasi modes in inviscid parallel shear flowsPoster presentation
- 日本惑星科学会2023年秋季講演会, Oct. 2023, Japanese, Hiroshima, Japan, Domestic conferenceDevelopment of weakly-compressible SPH method for simulating planetary mantle convectionPoster presentation
- Japan Geoscience Union Meeting 2023, May 2023, Japanese, Chiba, Japan, Domestic conferenceRevisit of the stability of inviscid horizontal shear flows with the method of spectral deformationPoster presentation
- Japan Geoscience Union Meeting 2022, Jun. 2022, Japanese, Chiba / online, Japan, Domestic conferenceImproving the DISPH method for simulating planetary core formationPoster presentation
- Japan Geoscience Union Meeting 2022, Jun. 2022, Japanese, Chiba / online, Japan, Domestic conferenceTwo-dimensional ideal MHD waves over a rotating sphere with continuous spectra of slow magnetic Rossby and Alfvén wavesPoster presentation
- Japan Geoscience Union Meeting 2021, Jun. 2021, Japanese, online, Japan, Domestic conferenceTwo-dimensional ideal MHD waves and the continuous Alfvén spectrum on a rotating sphere with a background toroidal magnetic fieldPoster presentation
- GFDオンラインセミナー 第3回, Dec. 2020, Japanese, オンライン, Japan連続モードの出現に着目した2次元回転球面上の磁気流体波動の解析Oral presentation
- JpGU-AGU Joint Meeting 2020:Virtual, Jul. 2020, English, online, Japan, Domestic conferenceContribution to IGRF-13 from Japan: A secular variation model using a numerical dynamo model and 4DEnVar data assimilationOral presentation
- JpGU-AGU Joint Meeting 2020:Virtual, Jul. 2020, Japanese, online, Japan, Domestic conferenceForecasts of geomagnetic secular variation using core surface flow models (2)Poster presentation
- JpGU-AGU Joint Meeting 2020:Virtual, Jul. 2020, English, online, Japan, Domestic conferenceInferring geomagnetic secular variation using MHD/kinematic dynamo modeling with data assimilationPoster presentation
- JpGU-AGU Joint Meeting 2020:Virtual, Jul. 2020, Japanese, online, Japan, Domestic conferenceShallow water MHD waves trapped in the polar regions on a rotating sphere with an imposed azimuthal magnetic fieldPoster presentation
- JpGU-AGU Joint Meeting 2020:Virtual, Jul. 2020, English, online, Japan, Domestic conferenceShallow water MHD waves trapped near the poles in a stably stratified outermost Earth's corePoster presentation
- 146th SGEPSS Fall Meeting (SGEPSS Fall Meeting 2019), Oct. 2019, Japanese, Kumamoto, Japan, Domestic conferenceShallow water MHD waves trapped in the polar regions on a rotating sphere with an imposed azimuthal magnetic fieldPoster presentation
- Japan Geoscience Union Meeting 2019, May 2019, Japanese, Chiba, Japan, Domestic conferenceTwo-dimensional or shallow water MHD waves on a rotating sphere with an imposed azimuthal magnetic fieldPoster presentation
- Workshop: Forecasting the geomagnetic secular variation with data assimilation, Sep. 2018, English, Paris, France, International conferenceEffects of an azimuthal background magnetic field on slow waves in a stably stratified outermost Earth's coreOral presentation
- Japan Geoscience Union Meeting 2018, May 2018, English, Chiba, Japan, Domestic conferenceThe effect of an azimuthal background magnetic field on waves in a stably stratified layer at the top of the Earth's outer corePoster presentation
- 第49回 地磁気・古地磁気・岩石磁気 夏の学校, Sep. 2017, Japanese, 福岡, Japan地球外核最上部の安定成層における流体波動 〜地磁気永年変動との比較に向けて〜Oral presentation
- JpGU-AGU Joint Meeting 2017, May 2017, Japanese, Chiba, Japan, Domestic conferenceEquatorial waves modified by the presence of a toroidal magnetic field within the stably stratified layer at the top of the Earth’s outer corePoster presentation
- 地球流体セミナー 分科会, Aug. 2016, Japanese, 北海道 支笏湖, JapanAlfvén波の固有モード 〜単純かと思いきや、ちょっと困った〜Others
- Japan Geoscience Union Meeting 2016, May 2016, Japanese, Chiba, Japan, Domestic conferenceThe empirical mode analysis of the decadal variations in the geomagnetic Gauss coefficientsPoster presentation
- Japan Symposium of Study of the Earth’s Deep Interior 2015, Sep. 2015, English, Tokyo, Japan, Domestic conferenceThe boundary mode of the axially symmetric MAC wave in the stratified layer at the top of the Earth’s outer corePoster presentation
- Japan Geoscience Union Meeting 2015, May 2015, Japanese, Chiba, Japan, Domestic conferenceThe boundary mode of axially symmetric MAC waves can exist in the stratified layer at the top of the Earth's outer corePoster presentation
- The Japan Society of Fluid MechanicsApr. 2026 - Present
- Society of Geomagnetism and Earth, Planetary and Space SciencesMay 2025 - Present
- The Japanese Society for Planetary SclencesJul. 2024 - Present
- Division of Plasma Physics Association of Asia Pacific Physical SocietiesMay 2024 - Present
- Japan Geoscience UnionFeb. 2015 - Present
■ Research Themes
- 日本学術振興会, 科学研究費助成事業, 若手研究, 九州大学, Apr. 2025 - Mar. 2029, Principal investigator地球外核最上部のダイナミクス:波が駆動する大規模地磁気変動の観測可能性の検証
- 日本学術振興会, 科学研究費助成事業, 基盤研究(B), 神戸大学, Apr. 2024 - Mar. 2028, Coinvestigator惑星内部ダイナモから表層大気雲対流までを包括した木星変動現象の解明
- 九州大学 応用力学研究所 共同利用・共同研究, Apr. 2026 - Mar. 2027, Principal investigator地球外核最上部を伝播する磁気流体波の連続スペクトル減衰とその数値シミュレ ーション
- 日本学術振興会, 科学研究費助成事業, 基盤研究(C), 九州大学, Apr. 2024 - Mar. 2027, Coinvestigator地球外核最上部のダイナミクス:波動による地球内部東西磁場強度推定の試み
- 九州大学 応用力学研究所 共同利用・共同研究, Apr. 2025 - Mar. 2026, Principal investigator地球外核最上部を伝播する磁気流体波の連続スペクトル減衰
- 核融合科学研究所 一般共同研究, Apr. 2024 - Mar. 2025, Principal investigator地球外核最上部におけるアルフベン波連続スペクトル
- 九州大学 博士後期課程奨学金, Jul. 2017 - Mar. 2020地球外核最上部の安定成層内の流体波動に関する研究
■ Others
