Takanobu Amano
Associate Professor
Department of Earth and Planetary Science,
Graduate School of Science, The University of TokyoPERSONAL DETAILS
Affiliation

Department of Earth and Planetary Science,
Graduate School of Science, The University of Tokyo

Address

Room 803, Faculty of Science Bldg. 1,
7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, JAPAN.

E-mailamano@eps.s.u-tokyo.ac.jp

Phone+81–3–5841–1921

Fax+81–3–5841–8321

Websitehttps://amanotk.github.io/

RESEARCH INTERESTS
Takanobu Amano is interested in theoretical aspects of space and astrophysical plasma
phenomena. His major research interests include physics of collisionless shocks (bothnon-relativistic and relativistic regimes), high-energy particle acceleration and transport, linear and nonlinear theory for kinetic plasma instabilities, and numerical techniques for advanced kinetic/fluid plasma simulations.

APPOINTMENTS
Aug. 1, 2016 - present

Associate Professor
Department of Earth and Planetary Science,
School of Science, The University of Tokyo

Mar. 16, 2012 - Jul. 31, 2016

Assistant Professor
Department of Earth and Planetary Science,
School of Science, The University of Tokyo

Apr. 1, 2009 - Mar. 15, 2012

Designated Assistant Professor
Division of Particle and Astrophysical Science,
Nagoya University

Apr. 1, 2008 - Mar. 31, 2009

Postdoctoral Researcher
Solar-Terrestrial Environment Laboratory,
Nagoya University

EDUCATION
Apr. 1, 2005 - Mar. 31, 2008

Ph.D degree
Department of Earth and Planetary Science,
Graduate School of Science, The University of Tokyo

Apr. 1, 2003 - Mar. 31, 2005

MS degree
Department of Earth and Planetary Science,
Graduate School of Science, The University of Tokyo

Apr. 1, 1999 - Mar. 31, 2003

BS degree
Department of Earth and Planetary Physics,
School of Science, The University of Tokyo

AWARDS• 2022 Tanakadate Award from from Society of Geomagnetism and Earth, Planetary
and Space Sciences (SGEPSS)• 2018 Young Researcher Award (under 40 yrs. old) from Association of Asia PacificPhysical Societies, Division of Plasma Physics (AAPPS-DPP)• 2015 Obayashi Early Career Scientist Award from Society of Geomagnetism andEarth, Planetary and Space Sciences (SGEPSS)• 2005 JSPS (Japan Society for the Promotion of Science) Research Fellowship for
Young Scientists (DC1)

PUBLICATIONS
See also, Google Scholar, or Publons profile pages for the up-to-date list of publications
and citation statistics.

Refereed Articles[1] Amano, T., M. Masuda, M. Oka, N. Kitamura, O. Le Contel, and D. J. Gershman(2024). Statistical Analysis of High-Frequency Whistler Waves at Earth’s Bow Shock:
Further Support for Stochastic Shock Drift Acceleration. Physics of Plasmas 31(4),042903. https://doi.org/10.1063/5.0196502[2] Jikei, T. and T. Amano (2024). Saturation Level of Ion Weibel Instability andIsotropization Length-Scale in Electron–Ion Weibel-mediated Shocks. Monthly
Notices of the Royal Astronomical Society 531(1), 219–229. https://doi.org/10.
1093/mnras/stae1187[3] Lindberg, M., A. Vaivads, T. Amano, S. Raptis, and S. Joshi (2024). Electron Acceleration at Earth’s Bow Shock Due to Stochastic Shock Drift Acceleration. GeophysicalResearch Letters 51(5), e2023GL106612. https://doi.org/10.1029/2023GL106612[4] Boula, S. S., J. Niemiec, T. Amano, and O. Kobzar (2024). Quasi-Perpendicular
Shocks of Galaxy Clusters in Hybrid Kinetic Simulations: The Structure of the
Shocks. Astronomy & Astrophysics 684, A129. https://doi.org/10.1051/0004-6361/
202349091[5] Jikei, T., T. Amano, and Y. Matsumoto (2024). Enhanced Magnetic Field Amplification by Ion-beam Weibel Instability in Weakly Magnetized Astrophysical Shocks.
The Astrophysical Journal 961(2), 157. https://doi.org/10.3847/1538-4357/ad1594[6] Iwamoto, M., Y. Matsumoto, T. Amano, S. Matsukiyo, and M. Hoshino (2024). Linearly Polarized Coherent Emission from Relativistic Magnetized Ion-Electron
Shocks. Physical Review Letters 132(3), 035201. https://doi.org/10.1103/PhysRevLett.
132.035201[7] Yamakawa, T., K. Seki, T. Amano, Y. Miyoshi, N. Takahashi, A. Nakamizo, andK. Yamamoto (2023). Effects of Cold Plasma on the Excitation of Internally Driven
ULF Waves by Ring Current Ions Based On the Magnetosphere-Ionosphere Coupled
Model. Journal of Geophysical Research: Space Physics 128(9). https://doi.org/
10.1029/2023JA031638[8] Raymond, J. C., P. Ghavamian, A. Bohdan, D. Ryu, J. Niemiec, L. Sironi, A. Tran,
E. Amato, M. Hoshino, M. Pohl, T. Amano, and F. Fiuza (2023). Electron–Ion Temperature Ratio in Astrophysical Shocks. The Astrophysical Journal 949(2), 50.
https://doi.org/10.3847/1538-4357/acc528[9] Kuramitsu, Y., Y. Matsumoto, and T. Amano (2023). Nonlinear Evolution of theWeibel Instability with Relativistic Laser Pulses. Physics of Plasmas 30(3), 032109.
https://doi.org/10.1063/5.0138855[10] Kitamura, N., T. Amano, Y. Omura, S. A. Boardsen, D. J. Gershman, Y. Miyoshi,
M. Kitahara, Y. Katoh, H. Kojima, S. Nakamura, M. Shoji, Y. Saito, S. Yokota, B. L. Giles,
W. R. Paterson, C. J. Pollock, A. C. Barrie, D. G. Skeberdis, S. Kreisler, O. Le Contel,
C. T. Russell, R. J. Strangeway, P.-A. Lindqvist, R. E. Ergun, R. B. Torbert, and J. L.
Burch (2022). Direct Observations of Energy Transfer from Resonant Electrons toWhistler-Mode Waves in Magnetosheath of Earth. Nature Communications 13(1),6259. https://doi.org/10.1038/s41467-022-33604-2[11] Amano, T. and M. Hoshino (2022). Theory of Electron Injection at Oblique Shockof Finite Thickness. The Astrophysical Journal 927(1), 132. https://doi.org/10.
3847/1538-4357/ac4f49[12] Yamakawa, T., K. Seki, T. Amano, Y. Miyoshi, N. Takahashi, A. Nakamizo, andK. Yamamoto (2022). Excitation of Two Types of Storm-Time Pc5 ULF Waves
by Ring Current Ions Based on the Magnetosphere-Ionosphere Coupled Model.
Journal of Geophysical Research: Space Physics 127(8). https://doi.org/10.1029/
2022JA030486[13] Walia, N. K., K. Seki, and T. Amano (2022). Study of Slow-mode Shock Formation and Particle Acceleration in the Symmetric Magnetic Reconnection Basedon Hybrid Simulations. Journal of Geophysical Research: Space Physics 127(5),e2021JA030066. https://doi.org/10.1029/2021JA030066[14] Jikei, T. and T. Amano (2022). Critical Comparison of Collisionless Fluid Models:Nonlinear Simulations of Parallel Firehose Instability. Physics of Plasmas 29(2),022102. https://doi.org/10.1063/5.0077064[15] Amano, T., Y. Matsumoto, A. Bohdan, O. Kobzar, S. Matsukiyo, M. Oka, J. Niemiec,
M. Pohl, and M. Hoshino (2022). Nonthermal Electron Acceleration at Collisionless
Quasi-Perpendicular Shocks. Reviews of Modern Plasma Physics 6(1), 29. https://doi.org/10.1007/s41614-022-00093-1[16] Iwamoto, M., T. Amano, Y. Matsumoto, S. Matsukiyo, and M. Hoshino (2022). Particle Acceleration by Pickup Process Upstream of Relativistic Shocks. The Astrophysical Journal 924(2), 108. https://doi.org/10.3847/1538-4357/ac38aa[17] Keika, K., S. Kasahara, S. Yokota, M. Hoshino, K. Seki, T. Amano, L. M. Kistler,
M. Nosé, Y. Miyoshi, T. Hori, and I. Shinohara (2022). Preferential Energizationof Lower-Charge-State Heavier Ions in the near-Earth Magnetotail. Journal ofGeophysical Research: Space Physics 127(1), e2021JA029786. https://doi.org/10.
1029/2021JA029786[18] Kobzar, O., J. Niemiec, T. Amano, M. Hoshino, S. Matsukiyo, Y. Matsumoto, and
M. Pohl (2021). Electron Acceleration at Rippled Low-Mach-number Shocks in
High-Beta Collisionless Cosmic Plasmas. The Astrophysical Journal 919(2), 97.
https://doi.org/10.3847/1538-4357/ac1107[19] Nishigai, T. and T. Amano (2021). Mach Number Dependence of Ion-Scale Kinetic
Instability at Collisionless Perpendicular Shock: Condition for Weibel-dominated
Shock. Physics of Plasmas 28(7), 072903. https://doi.org/10.1063/5.0051269 (Corresponding Author)[20] Kitamura, N., M. Shoji, S. Nakamura, M. Kitahara, T. Amano, Y. Omura, H. Hasegawa,
S. A. Boardsen, Y. Miyoshi, Y. Katoh, M. Teramoto, Y. Saito, S. Yokota, M. Hirahara,
D. J. Gershman, B. L. Giles, C. T. Russell, R. J. Strangeway, N. Ahmadi, P.-A. Lindqvist,
R. E. Ergun, S. A. Fuselier, and J. L. Burch (2021). Energy Transfer between Hot
Protons and Electromagnetic Ion Cyclotron Waves in Compressional Pc5 UltraLow Frequency Waves. Journal of Geophysical Research: Space Physics 126(5),e2020JA028912. https://doi.org/10.1029/2020ja028912

[21] Jikei, T. and T. Amano (2021). A Non-Local Fluid Closure for Modeling Cyclotron
Resonance in Collisionless Magnetized Plasmas. Physics of Plasmas 28(4), 042105.
https://doi.org/10.1063/5.0045335[22] Ligorini, A., J. Niemiec, O. Kobzar, M. Iwamoto, A. Bohdan, M. Pohl, Y. Matsumoto,T. Amano, S. Matsukiyo, and M. Hoshino (2021). Mildly Relativistic Magnetized
Shocks in Electron-Ion Plasmas - II. Particle Acceleration and Heating. Monthly
Notices of the Royal Astronomical Society 502(4), 5065–5074. https://doi.org/10.
1093/mnras/stab220[23] Bohdan, A., M. Pohl, J. Niemiec, P. J. Morris, Y. Matsumoto, T. Amano, M. Hoshino,
and A. Sulaiman (2021). Magnetic Field Amplification by the Weibel Instability at
Planetary and Astrophysical Shocks with High Mach Number. Physical Review
Letters 126(9), 095101. https://doi.org/10.1103/PhysRevLett.126.095101[24] Ligorini, A., J. Niemiec, O. Kobzar, M. Iwamoto, A. Bohdan, M. Pohl, Y. Matsumoto,T. Amano, S. Matsukiyo, Y. Esaki, and M. Hoshino (2021). Mildly Relativistic
Magnetized Shocks in Electron-Ion Plasmas - I. Electromagnetic Shock Structure.
Monthly Notices of the Royal Astronomical Society 501(4), 4837–4849. https://doi.org/10.1093/mnras/staa3901[25] Bohdan, A., M. Pohl, J. Niemiec, P. J. Morris, Y. Matsumoto, T. Amano, and M. Hoshino(2020). Kinetic Simulation of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. IV. Electron Heating. The Astrophysical Journal 904(1), 12.
https://doi.org/10.3847/1538-4357/abbc19[26] Yamakawa, T., K. Seki, T. Amano, N. Takahashi, and Y. Miyoshi (2020). Excitationof Internally Driven ULF Waves by the Drift-Bounce Resonance with Ring Current
Ions Based on the Drift-Kinetic Simulation. Journal of Geophysical Research: Space
Physics 125(11), e2020JA028231. https://doi.org/10.1029/2020ja028231[27] Kitamura, N., Y. Omura, S. Nakamura, T. Amano, S. A. Boardsen, N. Ahmadi, O. Le Contel, P. A. Lindqvist, R. E. Ergun, Y. Saito, S. Yokota, D. J. Gershman, W. R. Paterson,
C. J. Pollock, B. L. Giles, C. T. Russell, R. J. Strangeway, and J. L. Burch (2020). Observations of the Source Region of Whistler Mode Waves in Magnetosheath Mirror Structures. Journal of Geophysical Research: Space Physics 125(5). https://doi.org/10.1029/2019JA027488[28] Bohdan, A., M. Pohl, J. Niemiec, S. Vafin, Y. Matsumoto, T. Amano, and M. Hoshino(2020). Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. III. Magnetic Reconnection. The Astrophysical Journal 893(1),6. https://doi.org/10.3847/1538-4357/ab7cd6[29] Amano, T., T. Katou, N. Kitamura, M. Oka, Y. Matsumoto, M. Hoshino, Y. Saito,
S. Yokota, B. L. Giles, W. R. Paterson, C. T. Russell, O. Le Contel, R. E. Ergun, P.-A.
Lindqvist, D. L. Turner, J. F. Fennell, and J. B. Blake (2020). Observational Evidence
for Stochastic Shock Drift Acceleration of Electrons at the Earth’s Bow Shock.
Physical Review Letters 124(6), 065101. https://doi.org/10.1103/PhysRevLett.
124.065101[30] Oka, M., F. Otsuka, S. Matsukiyo, L. B. I. Wilson, M. R. Argall, T. Amano, T. D. Phan,
M. Hoshino, O. L. Contel, D. J. Gershman, J. L. Burch, R. B. Torbert, J. C. Dorelli, B. L.
Giles, R. E. Ergun, C. T. Russell, and P. A. Lindqvist (2019). Electron Scattering by LowFrequency Whistler Waves at Earth’s Bow Shock. The Astrophysical Journal 886(1),53. https://doi.org/10.3847/1538-4357/ab4a81

[31] Bohdan, A., J. Niemiec, M. Pohl, Y. Matsumoto, T. Amano, and M. Hoshino (2019).
Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova
Remnants. II. Influence of Shock-surfing Acceleration on Downstream Electron
Spectra. The Astrophysical Journal 885(1), 10. https://doi.org/10.3847/1538-4357/
ab43cf[32] Iwamoto, M., T. Amano, M. Hoshino, Y. Matsumoto, J. Niemiec, A. Ligorini, O. Kobzar,
and M. Pohl (2019). Precursor Wave Amplification by Ion–Electron Couplingthrough Wakefield in Relativistic Shocks. The Astrophysical Journal 883(2), L35.
https://doi.org/10.3847/2041-8213/ab4265[33] Bohdan, A., J. Niemiec, M. Pohl, Y. Matsumoto, T. Amano, and M. Hoshino (2019).
Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova
Remnants. I. Electron Shock-surfing Acceleration. The Astrophysical Journal 878(1),5. https://doi.org/10.3847/1538-4357/ab1b6d[34] Katou, T. and T. Amano (2019). Theory of Stochastic Shock Drift Acceleration forElectrons in the Shock Transition Region. The Astrophysical Journal 874(2), 119.
https://doi.org/10.3847/1538-4357/ab0d8a[35] Yamakawa, T., K. Seki, T. Amano, N. Takahashi, and Y. Miyoshi (2019). Excitationof Storm Time Pc5 ULF Waves by Ring Current Ions Based on the Drift-Kinetic
Simulation. Geophysical Research Letters 46(4), 1911–1918. https://doi.org/10.
1029/2018GL081573[36] Amano, T., M. Iwamoto, Y. Matsumoto, and M. Hoshino (2019). The Efficiency of
Coherent Radiation from Relativistic Shocks. Volume 119, pp. 371–383. Springer,Cham[37] Seki, K., Y. Miyoshi, Y. Ebihara, Y. Katoh, T. Amano, S. Saito, M. Shoji, A. Nakamizo,
K. Keika, T. Hori, S. Nakano, S. Watanabe, K. Kamiya, N. Takahashi, Y. Omura,
M. Nose, M.-C. Fok, T. Tanaka, A. Ieda, and A. Yoshikawa (2018). Theory, Modeling,and Integrated Studies in the Arase (ERG) Project. Earth, Planets and Space 70(1),17. https://doi.org/10.1186/s40623-018-0785-9[38] Keika, K., S. Kasahara, S. Yokota, M. Hoshino, K. Seki, M. Nosé, T. Amano, Y. Miyoshi,
and I. Shinohara (2018). Ion Energies Dominating Energy Density in the Inner
Magnetosphere: Spatial Distributions and Composition, Observed by Arase/MEP-i.
Geophysical Research Letters 45(22), 12,153–12,162. https://doi.org/10.1029/
2018GL080047[39] Amano, T. (2018). A Generalized Quasi-Neutral Fluid-Particle Hybrid Plasma Modeland Its Application to Energetic-Particle-Magnetohydrodynamics Hybrid Simulation. Journal of Computational Physics 366, 366–385. https://doi.org/10.1016/j.
jcp.2018.04.020[40] Walia, N. K. K., K. Seki, M. Hoshino, T. Amano, N. Kitamura, Y. Saito, S. Yokota,
C. J. J. Pollock, B. L. L. Giles, T. E. E. Moore, R. B. B. Torbert, C. T. T. Russell, andJ. L. Burch (2018). A Statistical Study of Slow-Mode Shocks Observed by MMS
in the Dayside Magnetopause. Geophysical Research Letters 45(10), 4675–4684.
https://doi.org/10.1029/2018GL077580[41] Iwamoto, M., T. Amano, M. Hoshino, and Y. Matsumoto (2018). Precursor Wave
Emission Enhanced by Weibel Instability in Relativistic Shocks. The AstrophysicalJournal 858(2), 93. https://doi.org/10.3847/1538-4357/aaba7a[42] Kamiya, K., K. Seki, S. Saito, T. Amano, and Y. Miyoshi (2018). Formation of Butterfly
Pitch Angle Distributions of Relativistic Electrons in the Outer Radiation Belt witha Monochromatic Pc5 Wave. Journal of Geophysical Research 123(6), 4679–4691.
https://doi.org/10.1002/2017JA024764[43] Matsumoto, Y., T. Amano, T. N. Kato, and M. Hoshino (2017). Electron Surfing andDrift Accelerations in a Weibel-Dominated High-Mach-Number Shock. Physical Review Letters 119(10), 105101. https://doi.org/10.1103/PhysRevLett.119.105101[44] Oka, M., L. B. I. Wilson, T. D. Phan, A. J. Hull, T. Amano, M. Hoshino, M. R. Argall,
O. L. Contel, O. Agapitov, D. J. Gershman, Y. V. Khotyaintsev, J. L. Burch, R. B. Torbert,
C. Pollock, J. C. Dorelli, B. L. Giles, T. E. Moore, Y. Saito, L. A. Avanov, W. Paterson, R. E.
Ergun, R. J. Strangeway, C. T. Russell, and P. A. Lindqvist (2017). Electron Scattering
by High-Frequency Whistler Waves at Earth’s Bow Shock. The AstrophysicalJournal 842(2), L11. https://doi.org/10.3847/2041-8213/aa7759[45] Iwamoto, M., T. Amano, M. Hoshino, and Y. Matsumoto (2017). Persistence ofPrecursor Waves in Two-Dimensional Relativistic Shocks. The Astrophysical Journal 840(1), 52. https://doi.org/10.3847/1538-4357/aa6d6f[46] Hirabayashi, K., M. Hoshino, and T. Amano (2016). A New Framework for Magnetohydrodynamic Simulations with Anisotropic Pressure. Journal of Computational
Physics 327, 851–872. https://doi.org/10.1016/j.jcp.2016.09.064[47] Amano, T. (2016). A Second-Order Divergence-Constrained Multidimensional
Numerical Scheme for Relativistic Two-Fluid Electrodynamics. The AstrophysicalJournal 831(1), 100. https://doi.org/10.3847/0004-637X/831/1/100[48] Balsara, D. S., T. Amano, S. Garain, and J. Kim (2016). A High-Order Relativistic TwoFluid Electrodynamic Scheme with Consistent Reconstruction of Electromagnetic
Fields and a Multidimensional Riemann Solver for Electromagnetism. Journal ofComputational Physics 318, 169–200. https://doi.org/10.1016/j.jcp.2016.05.006[49] Amano, T. (2015). Divergence-Free Approximate Riemann Solver for the QuasiNeutral Two-Fluid Plasma Model. Journal of Computational Physics 299, 863–886.
https://doi.org/10.1016/j.jcp.2015.07.035[50] Matsumoto, Y., T. Amano, T. N. Kato, and M. Hoshino (2015). Stochastic Electron
Acceleration during Spontaneous Turbulent Reconnection in a Strong Shock Wave.
Science (New York, N.Y.) 347(6225), 974–978. https://doi.org/10.1126/science.
1260168[51] Minoshima, T., Y. Matsumoto, and T. Amano (2015). A Finite Volume Formulationof the Multi-Moment Advection Scheme for Vlasov Simulations of Magnetized
Plasma. Computer Physics Communications 187, 137–151. https://doi.org/10.
1016/j.cpc.2014.10.023[52] Itou, H., T. Amano, and M. Hoshino (2014). First-Principles Simulations of Electrostatic Interactions between Dust Grains. Physics of Plasmas 21(12), 123707.
https://doi.org/10.1063/1.4904373[53] Amano, T., K. Higashimori, and K. Shirakawa (2014). A Robust Method for Handling
Low Density Regions in Hybrid Simulations for Collisionless Plasmas. Journal ofComputational Physics 275, 197–212. https://doi.org/10.1016/j.jcp.2014.06.048

[54] Matsumoto, Y., T. Amano, and M. Hoshino (2013). Electron Acceleration in a Nonrelativistic Shock with Very High Alfvén Mach Number. Physical Review Letters 111(21), 215003. https://doi.org/10.1103/PhysRevLett.111.215003[55] Saito, T., M. Hoshino, and T. Amano (2013). Stability of Cosmic-Ray Modified Shocks:
Two-Fluid Approach. The Astrophysical Journal 775(2), 130. https://doi.org/10.
1088/0004-637X/775/2/130[56] Amano, T. and J. G. Kirk (2013). The Role of Superluminal Electromagnetic Waves
in Pulsar Wind Termination Shocks. The Astrophysical Journal 770(1), 18. https://doi.org/10.1088/0004-637X/770/1/18[57] Minoshima, T., Y. Matsumoto, and T. Amano (2013). Multi-Moment Advection
Scheme in Three Dimension for Vlasov Simulations of Magnetized Plasma. Journalof Computational Physics 236, 81–95. https://doi.org/10.1016/j.jcp.2012.11.024[58] Matsumoto, Y., T. Amano, and M. Hoshino (2012). Electron Accelerations at HighMach Number Shocks: Two-Dimensional Particl-in-Cell Simulations in Various
Parameter Regimes. The Astrophysical Journal 755(2), 109. https://doi.org/10.
1088/0004-637X/755/2/109[59] Umeda, T., S. Matsukiyo, T. Amano, and Y. Miyoshi (2012). A Numerical Electromagnetic Linear Dispersion Relation for Maxwellian Ring-Beam Velocity d Istributions.
Physics of Plasmas 19(7), 072107. https://doi.org/10.1063/1.4736848[60] Hayakawa, T., K. Torii, R. Enokiya, T. Amano, and Y. Fukui (2012). Molecular andAtomic Gas toward HESS J1745-303 in the Galactic Center: Further Support for
the Hadronic Scenario. Publications of the Astronomical Society of Japan 64(1), 8.
https://doi.org/10.1093/pasj/64.1.8[61] Minoshima, T., Y. Matsumoto, and T. Amano (2012). Multi-Moment Advection
Scheme for Vlasov Simulations. ASP Conference Series 459(17), 277–282[62] Amano, T. and M. Hoshino (2012). Recent Progress in the Theory of Electron Injection in Collisionless Shocks. Volume 33, pp. 143–152. Springer Berlin Heidelberg[63] Amano, T., K. Torii, T. Hayakawa, and Y. Fukui (2011). Stochastic Accelerationof Cosmic Rays in the Central Molecular Zone of the Galaxy. Publications of the
Astronomical Society of Japan 63(6), L63–L66. https://doi.org/10.1093/pasj/63.
6.L63[64] Minoshima, T., Y. Matsumoto, and T. Amano (2011). Multi-Moment Advection
Scheme for Vlasov Simulations. Journal of Computational Physics 230(17), 6800–6823.
https://doi.org/10.1016/j.jcp.2011.05.010[65] Amano, T., K. Seki, Y. Miyoshi, T. Umeda, Y. Matsumoto, Y. Ebihara, and S. Saito(2011). Self-Consistent Kinetic Numerical Simulation Model for Ring Current
Particles in the Earth’s Inner Magnetosphere. Journal of Geophysical Research 116,
A02216. https://doi.org/10.1029/2010JA015682[66] Amano, T. and M. Hoshino (2010). A Critical Mach Number for Electron Injectionin Collisionless Shocks. Physical Review Letters 104(18), 181102. https://doi.org/
10.1103/PhysRevLett.104.181102[67] Shimada, N., M. Hoshino, and T. Amano (2010). Structure of a Strong Supernova
Shock Wave and Rapid Electron Acceleration Confined in Its Transition Region.
Physics of Plasmas 17(3), 032902. https://doi.org/10.1063/1.3322828

[68] Amano, T. and M. Hoshino (2009). Electron Shock Surfing Acceleration in Multidimensions: Two-Dimensional Particle-in-Cell Simulation of Collisionless Perpendicular Shock. The Astrophysical Journal 690(1), 244–251. https://doi.org/10.1088/
0004-637X/690/1/244[69] Amano, T., M. Hoshino, M. Hirahara, Y. Miyoshi, N. Terada, T. Mukai, and I. Shinohara (2009). Effect of Shock Angle on Fast and Direct Acceleration of Electrons inHigh Mach Number Quasi-Perpendicular Shocks. In AIP Conference Proceedings,
Tokyo (Japan), pp. 36–39. AIP[70] Amano, T. and M. Hoshino (2009). Nonlinear Evolution of Buneman Instability
and Its Implication for Electron Acceleration in High Mach Number Collisionless
Perpendicular Shocks. Physics of Plasmas 16(10), 102901. https://doi.org/10.
1063/1.3240336[71] Amano, T. and M. Hoshino (2007). Electron Injection at High Mach Number QuasiPerpendicular Shocks: Surfing and Drift Acceleration. The Astrophysical Journal 661(1), 190–202. https://doi.org/10.1086/513599

Book Chapters[1] Amano, T. (2023). Generalized Quasi-Neutral Hybrid-Kinetic Simulations. Spaceand Astrophysical Plasma Simulation, 313–336. https://doi.org/10.1007/978-3-031-11870-8_
10

Non-Refereed Articles[1] Amano, T. (2016). Inside a Plasma Shock. Physics 9, 117. https://doi.org/10.
1103/Physics.9.117

Non-refereed Articles in Japanese[1] 星野真弘, 天野孝伸 (2009), 宇宙における衝撃波粒子加速機構の新展開, 日本物理学会誌,
64(6), 421[2] 天野孝伸 (2009), 超新星残骸衝撃波における電子注入, 天文月報, 102(1), 9

INVITED TALKS (INTERNATIONAL CONFERENCES)[1] Electron injection via stochastic shock drift acceleration at quasi-perpendicular
shocks, Synergistic approaches to particle transport in magnetized turbulence:from the laboratory to astrophysics, Apr. 16, 2024.
[2] Theory, Simulation, and Observation for Electron Injection at Collisionless Shocks,
AOGS 19th Annual Meeting, Online, Aug. 1, 2022.
[3] Electron injection at shocks: Transition from stochastic shock drift acceleration
to diffusive shock acceleration, XXVIII Cracow EPIPHANY Conference on Recent
Advances in Astroparticle Physics, Online, Jan. 12, 2022.
[4] Connecting Injection and Subsequent Acceleration of Nonthermal Electrons at
Collisionless Oblique Shocks, The 30th International Toki Conference on Plasma
and Fusion Research (ITC30), Online, Nov. 16, 2021. (Plenary Talk)[5] Stochastic Shock Drift Acceleration as the Mechanism for Electron Injection into
Diffusive Shock Acceleration at Collisionless Shocks, 5th Asia-Pacific Conferenceon Plasma Physics (AAPPS-DPP2021), Online, Sep. 28, 2021.
[6] Particle Acceleration at Collisionless Shocks, 10th East-Asia Workshop on Laboratory, Space, Astrophysical Plasmas (EASW-10), Online, Aug. 16, 2021.
[7] Perspectives for Electron Heating and Acceleration at Collisionless Shocks, MMS
Spring 2021 Science Working Team Meeting, Online, Apr. 8, 2021.
[8] Non-thermal Particle Acceleration at Collisionless Shocks, Max Planck Princeton
Center Workshop, Göttingen, Germany, Jan. 22, 2020.
[9] Three-dimensional Particle-In-Cell Simulations for High Mach Number Collisionless Shocks, The 2nd Asia-Pacific Conference on Plasma Physics, Kanazawa, Japan,
Nov. 15, 2018.
[10] Nonthermal Electron Acceleration at Earth’s Bow Shock: Theory, Simulation and
Observation, The 13th International School/Symposium for Space Simulations(ISSS-13), Los Angeles, USA, Sep. 13, 2018.
[11] Stochastic Shock Drift Acceleration for Electrons, 8th East-Asia Workshop on Laboratory, Space, Astrophysical Plasmas, Daejeon, Korea, Aug. 1, 2018.
[12] Cosmic-Ray Acceleration via Astrophysical Coherent Radiation, 20th International
Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI), Nagoya,Japan, May 24, 2018.
[13] Particle Acceleration in Relativistic Plasmas, Dawn of a New Era for Black Hole
Jets in Active Galaxies, Sendai, Japan, Jan. 26, 2018.
[14] Nonthermal Electrons at Quasi-perpendicular Collisionless Shocks, 7th East-Asia
Workshop on Laboratory, Space, Astrophysical Plasmas, Weihai, China, Jul. 25,
2017.
[15] Coherent and Stochastic Acceleration in Quasi-perpendicular Collisionless Shocks,
Workshop on Plasma Astrophysics from the Laboratory to the Non-thermal Universe, Oxford, UK, Jul. 4, 2017.

[16] Kinetic Simulations of Particle Acceleration and Transport around Collisionless
Shocks, AOGS 13th Annual Meeting, Beijing, China, Aug. 1, 2016.
[17] Particle Acceleration and Transport at Collisionless Shocks, 6th East-Asia Workshop
on Laboratory, Space, Astrophysical Plasmas, Tsukuba, Japan, Jul. 11, 2016.
[18] Key Issues in Particle Acceleration Theory at Collisionless Shocks, 18th International Congress on Plasma Physics, Kaohsiung, Taiwan, Jun. 29, 2016.
[19] Energetic Particle Hybrid Code and Its Application, 11th International Conferenceon Numerical Modeling of Space Plasma Flows (ASTRONUM2016), Monterey, USA,
Jun. 9, 2016.
[20] Superluminal Electromagnetic Waves in Highly Magnetized Relativistic Shocks,
5th East-Asia School and Workshop on Laboratory, Space, Astrophysical Plasmas,
Pohang, Korea, Aug. 21, 2015.
[21] Quasi-neutral Two-fluid Plasma Simulation Model, 10th International Conferenceon Numerical Modeling of Space Plasma Flows (ASTRONUM 2015), Avignon, France,
Jun. 10, 2015.
[22] Physics of Very High Mach Number Collisionless Shocks, The Many Facets of Supernova Remnants, Rikkyo University, Japan, Nov. 10, 2014.
[23] Relativistic Electromagnetic Two-fluid Simulations of Pulsar Wind Termination
Shocks, The 6th East-Asian Numerical Astrophysics Meeting (EANAM6), Suwon,
Korea, Sep. 18, 2014.
[24] Robust Handling of Low Density Regions in Hybrid Simulations, 9th International
Conference on Numerical Modeling of Space Plasma Flows (ASTRONUM 2014),
Long Beach, USA, Jun. 25, 2014.
[25] Relativistic Pulsar Wind Termination Shocks Modified by Superluminal Electromagnetic Waves, 8th International Conference on Numerical Modeling of Space
Plasma Flows (ASTRONUM 2013), Biarritz, France, Jul. 1, 2013.
[26] Structure of Relativistic Shock Modified by Nonlinear Superluminal Waves, Nonlinear Waves and Chaos Workshop 9, La Jolla, USA, Mar. 7, 2013.
[27] Self-consistent Drift-kinetic Numerical Ring-current Modeling : Five-dimensional
Vlasov-Maxwell Approach, Inner Magnetosphere Coupling II (IMC II), Los Angeles,
USA, Mar. 20, 2012.
[28] Nonthermal Electron Acceleration and Injection in Collisionless Shocks, International Astrophysics Forum Alpbach (IAFA) 2011, Alpbach, Austria, Jun. 24, 2011.
[29] Kinetic and Self-consistent Numerical Modeling of the Terrestrial Inner Magnetosphere, 6th International Conference on Numerical Modeling of Space Plasma
Flows (ASTRONUM 2011), Valencia, Spain, Jun. 17, 2011.
[30] Electron Acceleration and Injection by Whistler Waves in Collisionless Shocks,
2010 International Space Plasma Symposium, Tinan, Taiwan, Jun. 28, 2010.
[31] Surfing and Drift Acceleration of Electrons at High Mach Number Quasi-perpendicular
Shocks, Kinetic Modeling of Astrophysical Plasmas, Crakow, Poland, Oct. 6, 2008.
[32] Nonthermal Electron Acceleration in High Mach Number Collisionless Shocks, The
9th International Workshop on the Interrelationship between Plasma Experiments
in Laboratory and Space (IPELS), Palm Cove, Australia, Aug. 10, 2007.

INVITED TALKS (DOMESTIC CONFERENCES)[1] 宇宙プラズマにおける運動論的不安定性, プラズマシミュレータシンポジウム, オンライン,
2023 年 9 月 28 日.
[2] ミクロなプラズマ素過程に基づく衝撃波粒子加速機構, 高エネルギー現象で探る宇宙の多様性Ⅰ, 東京大学宇宙線研究所, 2021 年 10 月 19 日.
[3] 衝撃波電子加速におけるホイッスラー波の役割, 第 37 回プラズマ・核融合学会年会シンポジウム, オンライン, 2020 年 12 月 1 日.
[4] 内部磁気圏における ULF 波動励起機構, 実験室・宇宙プラズマ研究集会, 東京大学本郷キャンパス, 2019 年 9 月 17 日.
[5] 宇宙空間衝撃波の遷移層, 日本物理学会 春季年会, 東京理科大学野田キャンパス, 2018 年 3月 24 日.
[6] 内部磁気圏 RC モデリングの新しい試み, 太陽地球圏環境予測のためのモデル研究の展望, 名
古屋大学東山キャンパス, 2017 年 1 月 27 日.
[7] MMS 衛星で見る無衝突衝撃波と電子加速, 高エネルギー宇宙物理学研究会, 青山学院大学相模原キャンパス, 2016 年 12 月 2 日.
[8] 宇宙プラズマのハイブリッドシミュレーション, 日本物理学会 2016 秋季年会, 金沢大学角間キャンパス, 2016 年 9 月 14 日.
[9] Theory and Simulations of Particle Acceleration in Collisionless Shocks, 高エネル
ギーガンマ線でみる極限宇宙 2015, 2016 年 1 月 14 日.
[10] パルサー風衝撃波と電磁波の相互作用, 高エネルギー宇宙物理学研究会, 九州大学西新プラ
ザ, 2014 年 11 月 25 日.
[11] 相対論的電磁変性衝撃波の構造と電磁エネルギー散逸, 日本物理学会 2013 春季年会, 広島大学, 2013 年 3 月 27 日.
[12] 無衝突衝撃波の数値シミュレーションと粒子加速, 宇宙流体力学のフロンティア, 京都大学,
2009 年 11 月 16 日.