Publications

 Publication with Peer Review(PIx15, Co-PIx30)

2021

[1] 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

[2] 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

[3] 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

[4] 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 

     doi:10.1051/0004-6361/202038900

     

2020

[5] 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

[6] 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

   

[7] 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

[8] 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.

     doi:10.3847/1538-4357/ab8ea9

[9] 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 

[10] 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

[11] 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 

[12] 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

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

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

       247,6

[14] 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

[15] 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

2019

[16] 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

[17] 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

[18]  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

2018

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

        Atmospheric and Solar-Terrestrial physics, Volume 180: doi: doi.org/10.1016/j.jastp.2017.08.035

[20]  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

[21]  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

[22]  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 

[23]  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

2017

[24]  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

[25]  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

[26]  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

2016

[27]  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 

[28] 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

   

[29] 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

2015

[30] 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

2014

[31]  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

[32] 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

[33] 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

2013

[34] 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

[35] 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

2012

[36] 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

[37] 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

[38] 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

[39] 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

2011

[40] 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

[41] S. Inoue, and Y. Morikawa. "Three-Dimensional Modeling of Solar Active Region", Plasma and Fusion

        Research, Volume 6, 2401067 

2010

[42] 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 

2009

[43] 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

 

[44] 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

2006

[45] 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

A Chapter in a Book

[1]   Satoshi INOUE  

       "Three-Dimensional 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

[1] 井上 諭

   "太陽光球面磁場から外挿される太陽コロナ磁場の3次元構造" 

    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 靖大

      “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 No.2 2011.1 第11号

 

[3] 井上 諭

      “太陽活動領域での太陽嵐発生のアセスメント

     NICTニュース, 2011 1月号 No.400