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 Publication with Peer Review(PIx16, Co-PIx34)


[50] Mykola Gordovskyy,  Philippa K. Browing, Kanya Kusano,  Satoshi Inoue and​ Grigory E. Vekstein "Particle  

        Acceleration and Their  Escape into the Heliosphere in Solar Flares with Open Magnetic Field", The  

        Astrophysical Jpurnal 952 75

[49] Nian Liu, Ju Jing, Qiang Hu, Satoshi Inoue, Haimin Wang​ "The Initiation and Back-reaction of the X5.4

        Flare on 2012 Mach  7", The Astrophysical Journal 946 64

[48] Satoshi Inoue,  Keiji Hayashi, & Takahiro Miyoshi  "An Evolution and Eruption of the Coronal Magnetic

        Field through a Data-Driven MHD Simulation", The Astrophysical Journal, 946, 46 

[47] Satoshi Inoue,  Keiji Hayashi, Takahiro Miyoshi, Ju Jing, & Haimin Wang "A Comparative Study of Solar

       Active Region with Data-constrained and Data-driven MHD Simulations", The Astrophysical Journal

       Letters, 944, L44 doi:10.3847/2041-8213/acb7f4


[46] Daiki Yamasaki, Satoshi Inoue,  Yumi Bamba, Jeongwoo Lee, & Haimin Wang  " A Data-constrained

       Magnetohydrodynamic Simulation of the X1.0 Solar Flare of 2021 October 28, The Astrophysical

        Journal, 940, 119. doi: 10.3847/1538-4357/ac9df4

[45] Vasyl Yurchyshyl, Xu Yang, Gelu Nita, Gregory Fleishmann, Valentina Abramenko, Satoshi Inoue, 

        Eun-Kyung Lim, & Wenda Cao "Magnetic Field Re-configuration Associated With a Slow Rise Eruptive

           X1.2 Flare in NOAA Active Region 11944", Frontiers in Astronomy and, Space Sciences, 9(816523).



[44] Ju Jing, Satoshi Inoue,  Jeongwoo Lee, Qin Li, Gelu, Nita M, Yan Xu, Chang Liu, Dale Gary E, & Haimin

        Wang  "Understanding the Initiation of the M2.4 Flare on 2017 July 14 ", The Astrophysical Journal,

        922, 108. doi: 10.3847/1538-4357/ac26c7

[43] Satoshi Inoue & Yumi Bamba

       "An MHD Modeling of Successive X2.2 and X9.3 Flares of 2017 September ", 

        The Astrophysical Journal, 914, 71. doi:10.3847/1538-4357/abf835

[42] Daiki Yamasaki, Satoshi Inoue,  Shin-ichi Nagata, & Kiyoshi Ichimoto "Evolution of Nontential Magnetic

        Field  in Solar Active Region 12673 Based on a Nonlinear  Force-free Modeling", The Astrophysical

        Journal, 908, 132. doi:10.3847/1538-4357/abcfbb

[41] G. J. M. Vissers, S. Danilovic, J, de la Cuuz Rodriguez, J. Leenaarts, Moron, R., C. J. Daiu Baso, 

       A. Reid, D. J. Price, &  S. Inoue, "Non-LTE Inversions of a Confined X2.2 Flare: I. Vector Magnetic Field

       in the Photosphere and  Chromosphere", The Astronomy & Astrophysics, 645, A1 




[40] Mykola Gordovskyy, Philippa Browning K., Satoshi Inoue,  Eduard Kontar P., Kanya Kusano, & Grigory 

        Vekstein E. "Forward Modeling of Particle Acceleration and Transport in an Individual Solar Flare", 

        The Astrophysical Journal, 902, 147. doi:10.3847/1538-4357/abb60e

[39] Kanya Kusano, Tomoya Iju, Yumi Bamba, & ,  Satoshi Inoue, "A Physics-Based Method That Can Predict

        Imminent Large Solar Flares ", Science, 369 587-591 doi:10.1126/science.aaz2511


[38] Yusuke Kawabata, Andres Asensio Ramos, Satoshi Inoue,  & Toshifumi Shimizu "Chromospheric Magnetic

        Field: A Comparison of He I 10830 Å Observations with Nonlinear Force-Free Field Extrapolation", The

        Astrophysical  Journal, 898, 32. doi:10.3847/1538-4357/ab9816

[37] Y. Kawabata, S. Inoue, & T. Shimizu "Extrapolation of Three Dimensional Magnetic Field Structure in

       Flare-Productive Active Regions with Different Initial Condition", The Astrophysical Journal, 895, 105.


[36] Sergei Zharkov,  Sarah Matthews, Valentina Zharkova, Malcolm Druett, Satoshi Inoue, Ingolf    

        Dammasch, and Connor Macrae  "Sunquake with a Second-bounce, Other Sunquakes and Emission

       Associated  with X9.3  Flare of 6 September 2017. I. Observations", Astronomy & Astrophysics, 639,            A78 

[35] Valentina Zharkova, Sergei Zharkov, Malcolm Druett, Sarah Matthews, & Satoshi Inoue, 

       "Sunquake with a Second-bounce, Other Sunquakes and Emission Associated  with

       X9.3  Flare of 6 September 2017. II. Proposed Interpretation", Astronomy & Astrophysics, 639, A79

[34] Yumi Bamba, Satoshi Inoue, & Shinsuke Imada "Intrusion of a Magnetic Peninsula Toward the

        Neighboring Opposite-polarity Region That Triggers the Largest Solar Flare in Solar Cycle 24",          

        The Astrophysical Journal, 894, 29 

[33] Pei Hsuan Lin, Kanya Kusano, Daikou Shiota, Satoshi Inoue, K. D. Leka, & Yuta Mizuno. "A New Parameter

       of Photospheric  Magnetic Field to Determine Eruptive-Flare Producing Solar Active Region", The

       Astrophysical Journal 894, 20

[32] Takahiro Miyoshi, Kanya Kusano, & Satoshi Inoue. "A Magnetohydrodynamic Relaxation  Method for Non

       -Force-Free Magnetic Field  in Magnetohydrostatic Equilibrium", The Astrophysical Journal Supplement,


[31] Shin Torium, Shinsuke Takasao, Mark C. M. Cheung, Chaowei Jiang, Yang Guo, Keiji Hayashi, & Satoshi

       Inoue. "Comparative Study of Data-driven Solar  Coronal  Field Models Using a Flux Emergence

       Simulation as a Ground-truth Data Set", The Astrophysical Journal, 890, 103

[30] Magnus M. Woods, Satoshi Inoue , Louise K. Harra, Sarah A. Matthews, Kanya Kusano. "Serial Flaring in

       an Active Region: Exploring Why Only One Flare is Eruptive",The  Astrophysical Journal,  890, 84


[29] Jihye Kang, Satoshi Inoue, Kanya Kusano, Sung-Hong Park & Yong-Jae Moon. "Onset Mechanism of M6.5

        Flare Observed in Active Region 12371", The Astrophysical Journal, Volume 887, Issue 2, article  id.

        263, 8 pp. doi:10.3847/1538-4357/ab5582

[28] Yumi Bamba, Satoshi Inoue, & Keiji Hayashi. "The Role of Tiny Brightening in a Huge Geo-effective

       Solar Eruption Leading to the St Patrick's Day Storm", The Astrophysical Journal, Volume 874, Issue 1,

       article id. 73, 11 pp. doi:10.3847/1538-4357/ab06ff

[27]  Navin Chandra Joshi, Xiaoshuai Zhu, Brigitte Schmieder, Guillaume Aulanier, Miho Janvier,  Bhuwan

        Joshi, Tetsuya Magara, Ramesh Chandra, and  Satoshi Inoue. "Generalization of the Magnetic Field

        Configuration of Typical and  Atypical Confined Flare" The Astrophysical Journal, Volume 871, Issue 2,           id 165, 17pp doi:10.3847/1538-4357/aaf3b5


[26]  Satoshi Inoue, Yumi Bamba, and Kanya Kusano. "Onset Mechanism of the Solar Eruption " Journal of    

        Atmospheric and Solar-Terrestrial physics, Volume 180: doi:

[25]  Satoshi Inoue, Daikou Shiota, Yumi Bamba, and Sung-Hong Park. "Magnetohydrodynamic Modeling of

        a Solar Eruption Associated with X9.3 Flare Observed in Active Region 12673", The

        Astrophysical Journal, Volume 867, issue 1, id 83, doi:10.3847/1538-4357/aae079

[24]  Johan Muhamad, Kanya Kusano, Satoshi Inoue, and Yumi Bamba. "A Study of Magnetic Field

        Characteristics of Flaring Active Region Based on Nonlinear Force-Free Field Extrapolation" The    

        Astrophysical Journal, Volume 863, Issue 2, id 162

[23]  Magnus M. Woods, Satoshi Inoue , Louise K. Harra, Sarah A. Matthews, Kanya Kusano and Nadine M. E.

        Kalmoni. "The  Triggering of the 2014 March 29 Filament Eruption" The Astrophysical Journal, Volume           860, Issue 2, id 163 

[22]  Satoshi Inoue,  Kanya Kusano, Jörg Büchner, and Jan Skala. "Formation and Dynamics of a Solar

        Eruptive Flux Tube" Nature Communications, 9 174 doi:10.1038/s41467-017-02616-8


[21]  J. Muhamad, K. Kusano, S. Inoue and D. Shiota. "Magnetohydrodynamic Simulation for Studying Solar

        Flare Trigger Mechanism " The Astrophysical Journal, Volume 842, Issue 2, id 86

[20]  Y. Kawabata, S. Inoue, and T. Shimizu​. "Non-Potential Field Formation in X-Shaped Quadrupole

        Magnetic Field Configuration" The Astrophysical Journal, Volume 842, Issue 2, id 106

[19]  Yumi Bamba, Satoshi Inoue, Kanya Kusano, and Daikou Shiota. "Triggering Process of the X1.0 Three-

        Ribbon Flare in the Giant Active Region NOAA 12192" The Astrophysical Journal, Volume 838, Issue 2,           id


[18]  Jihye Kang, Tetsuya Magara, Satoshi Inoue, Yuki Kubo, and Naoto Nishizuka. "Distribution

        Characteristics of Electric Current Density as an Indicator for the Occurrence of a  Solar Flare",

        Publications of the Astronomical Society of Japan, Volume 68, Issue 6, id 101 

[17] S. Inoue. "Magnetohydrodynamics Modeling of Coronal Magnetic Field and Solar Eruptions Based on

        Photospheric Magnetic Field" Progress in Earth and Planetary Science, Volume  3, issue 1, article id

        19(Invited Reviewdoi: 10.1186/s40645-016-0084-7


[16] S. Inoue, K. Hayashi, and K. Kusano. "Structure and Stability of Magnetic Fields in Solar Active Region

        12192 Based on the Nonlinear Force-free Field Modeling" The Astrophysical Journal, Volume 818, issue

        2, id 168 doi: 10.3847/0004-637X/818/2/168


[15] S. Inoue, K. Hayashi, T. Magara, G. S. Choe, and Y. D. Park. "Magnetohydrodynamic Simulation of the

       X2.2 Solar Flare on 2011 February: II Dynamics Connecting the Solar Flare and the Coronal Mass

       Ejection" The Astrophysical Journal, Volume 803, Issue 2, id 73 doi: 10.1088/0004-637X/803/2/73


[14]  Navin Chandra Joshi, Tetsuya Magara, and Satoshi Inoue.“Formation of Composed Flux Rope by the

        Merging of Two Filament Channels Associated Dynamics and its Stability", The Astrophysical Journal,

        Volume 795, Issue 1, id 4

[13] S. Inoue, K. Hayashi, T. Magara, G. S. Choe, and Y. D. Park. "Magnetohydrodynamic Simulation of the

       X2.2 Solar Flare on 2011 February: I Comparison with the Observations" The Astrophysical Journal,

       Volume 788, Issue 2, id 182 doi: 10.1088/0004-637X/788/2/182

[12] S. Inoue, T. Magara, V. S. Pandey, D. Shiota, K. Kusano & G. S. Choe, and K. S. Kim. "Nonlinear Force-Free        Extrapolation of the Coronal Magnetic Field Based on the MHD-Relaxation Method" The Astrophysical

       Journal, Volume 780, Issue 1, id 101 doi: 10.1088/0004-637X/780/1/101


[11] S. Toriumi, Y. Iida, Y. Bamba, K. Kusano, S. Imada, and S. Inoue. "Magnetic Systems Triggering the

       M6.6-class Solar Flare in NOAA Active Region 11158", The Astrophysical Journal, Volume 773, Issue 2,

       id 128

[10] S. Inoue, K. Hayashi, D. Shiota, T. Magara, and G. S. Choe. "Magnetic Structure Producing X- and M-

       class Solar Flares in Solar Active Region 11158"The Astrophysical Journal, Volume 770, Issue 1, id 79 

       doi: 10.1088/0004-637X/770/1/79


[9] T. Magara, J. M. An, H. H. Lee, J. H. Kang, S. Inoue and G. S. Choe. "Chromospheric Running Wave

        Produced through the Emergence of a Twist Magnetic Flux Tube", Publications of the Astronomical

       Society of Japan, Volume 64, Issue 5,  L4

[8] S. Inoue, D. Shiota, T. T. Yamamoto, V. S. Pandey, T. Magara, and G. S. Choe. "Buildup and Release of

       Magnetic Twist During the X3.4 Solar Flare of 2006 December 13" The Astrophysical Journal, Volume

       760, Issue 1, id 17 doi: 0.1088/0004-637X/760/1/17

[7] S. Inoue, T. Magara, S. Watari, and G. S. Choe. "Non-Linear Force-Free Modeling of a Three-dimensional

       Sigmoid Observed on the Sun" The Astrophysical Journal, Volume 747, Issue 1, id 65 

       doi: 10.1088/0004-637X/747/1/65

[6] K. Iwai, Y. Miyhoshi, S. Masuda, M. Shimojo, D. Shiota, S. Inoue, A. Tsutiya, A. Morioka, and H. Misawa

       "Solar Radio Type-1 Noise Storm Modulated by Coronal Mass Ejections", The Astrophysical Journal,

       Volume 744, Issue 2, id 167


[5] S. Inoue, K. Kusano, T. Magara, D. Shiota, and T. T. Yamamoto. Twist and Connectivity of Magnetic Field

        Lines in the Solar Active Region NOAA 10930", The Astrophysical Journal, Volume 738, Issue 2, id 16 

        doi: 10.1088/0004-637X/738/2/161


[4] T. T. Yamamoto, R. Kataoka, and S. Inoue. "Helical Length of Magnetic Clouds From the Magnetic Flux

        Conservation ", The Astrophysical Journal, Volume 710, Issue 1, p456-461 


[3] R. Kataoka, T. Ebisuzaki, K. Kusano, D. Shiota, S. Inoue, T. T. Yamamoto, and M. Tokumaru. "Three-

       dimensional MHD modeling of the solar wind structures associated with 13 December 2006 coronal mass

       ejections", Journal of Geophysical Research, Volume 710, Issue 114, id 10102


[2] T. Minoshima, S. Imada, T. Morimoto, H. Koshiishi, M. Kubo, S. Inoue, H. Isobe, S. Masuda, S. Kurucker, 

        and T. Yokoyama. "Multi wavelength Observation of Electron Acceleration in 2006 December 13 Flare",

       The AstrophysicalJournal, Volume 697, Issue 1, p843-849


[1] S. Inoue, and K. Kusano."Three-Dimensional Simulation Study of Flux Rope Dynamics in the Solar

       Corona", The Astrophysical Journal, Volume 645, Issue 1, Page 742-756 

       doi: 10.1086/503153

 Conference  Proceedings

[1] S. Inoue & Y. Morikawa. "Three-dimensional Modeling of Solar Active Region", Plasma and Fusion

     Research, Volume 6, 2401067

 Chapter of a Book

[1] Satoshi Inoue  "Three-dimensional Modeling Coronal Magnetic Field Based on Photospheric Magnetic Field

     by Hinode/SP Observation" (Chapter 11), First Ten-years of Hinode on-Orbit Observatory, Editing  

     T. Shimizu, S. Imada, M. Kubo, Astrophysics and Space Science Library, Volume 449, p115-p119,

     Springer (2018) DOI:10.1007/978-981-10-7742-5_17

Japanese Articles (日本語)

[3] 井上 諭


   天文月報、第109巻9号 2016年9月号、「ひので10周年記念特集」

[2] 井上 諭、森川 靖弘

  "NICT 宇宙天気クラウドを用いた太陽活動領域磁場の再現" 

   大阪大学サイバーメディアセンター 計算機利用ニュース Vol.6 No2 2011.1 第11号

[1] 井上 諭


   NICTニュース、2011 1月号 No.400

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