Publications of Satoshi Inoue

A list of publications authored or co-authored by Satoshi Inoue, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0001-5121-5122

List of publications ordered by citations
Number of papers: 23 (refereed: 23)
No. of citations: 179
First author papers: 4 (refereed: 4)

2026

1. Stereoscopic Observations of Solar X-Ray Sources Explained by a Data-constrained Magnetohydrodynamic Simulation [0]
   Matsumoto, Keitarou, Inoue, Satoshi, Wang, Meiqi, Krucker, Säm, Masuda, Satoshi, Stiefel, Muriel Zoë, Lee, Jeongwoo, Chen, Bin & Wang, Haimin, ApJ, 998, L28
2. Driving Mechanisms of Solar Active Region Geysers: The Role of Interacting Magnetic Flux [0]
   Monga, Aabha, Inoue, Satoshi, Lee, Jeongwoo, Wang, Haimin & Hansteen, Viggo, ApJ, 996, L6
3. Large Magnetic Flux Rope Formation in an X2.1 Flare Observed on 2011 September 6 [0]
   Roddanavar, Arpita, Inoue, Satoshi, Hayashi, Keiji, Jing, Ju, Cao, Wenda & Wang, Haimin, ApJ, 997, 51
4. Finite Plasma β Three-dimensional Magnetic Field Extrapolation Based on the Magnetohydrodynamic Relaxation Method [0]
   Yamasaki, Daiki, Miyoshi, Takahiro & Inoue, Satoshi, ApJS, 282, 66

2025

1. Acceleration of Solar Eruptions via Enhanced Torus Instability Driven by Small-scale Flux Emergence [1]
   Inoue, Satoshi, Miyoshi, Takahiro, Hayashi, Keiji, Minh Triet Nguyen, Huu, Jing, Ju, Cao, Wenda & Wang, Haimin, ApJ, 988, L36
2. Mystery behind the Peeling of a Filament and the Associated Sudden Disappearance of a Sunspot Penumbra [0]
   Jing, Ju, Mancuso, Mia, Inoue, Satoshi, Lee, Jeongwoo, Li, Qin, He, Wen, Xu, Yan, Cao, Wenda & Wang, Haimin, ApJ, 993, L47
3. Data-constrained Magnetohydrodynamic Simulation for Magnetic Flux Rope Eruptions Driven by Magnetic Reconnection [5]
   Liu, Nian, Inoue, Satoshi, Wang, Ying & Wang, Haimin, ApJ, 983, 38
4. A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare [1]
   Matsumoto, Keitarou, Inoue, Satoshi, Hayashi, Keiji, Liu, Nian, Wang, Ying, Lee, Jeongwoo, Jing, Ju & Wang, Haimin, ApJ, 991, 77
5. A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. I. Dynamics of the Solar Eruption Associated with the X7.1 Solar Flare [3]
   Matsumoto, Keitarou, Inoue, Satoshi, Liu, Nian, Hayashi, Keiji, Jing, Ju & Wang, Haimin, ApJ, 985, 20

2024

1. Magnetic Eruption from a Three-ribbon Flare [2]
   Jing, Ju, Lee, Jeongwoo, Mancuso, Mia, Li, Qin, Liu, Nian, Inoue, Satoshi, Xu, Yan & Wang, Haimin, ApJ, 972, 110

2023

1. Particle Acceleration and Their Escape into the Heliosphere in Solar Flares with Open Magnetic Field [6]
   Gordovskyy, Mykola, Browning, Philippa K., Kusano, Kanya, Inoue, Satoshi & Vekstein, Grigory E., ApJ, 952, 75
2. An Evolution and Eruption of the Coronal Magnetic Field through a Data-driven MHD Simulation [13]
   Inoue, Satoshi, Hayashi, Keiji & Miyoshi, Takahiro, ApJ, 946, 46
3. A Comparative Study of Solar Active Region 12371 with Data-constrained and Data-driven Magnetohydrodynamic Simulations [12]
   Inoue, Satoshi, Hayashi, Keiji, Miyoshi, Takahiro, Jing, Ju & Wang, Haimin, ApJ, 944, L44
4. The Initiation and Back-reaction of the X5.4 Flare on 2012 March 7 [3]
   Liu, Nian, Jing, Ju, Hu, Qiang, Inoue, Satoshi & Wang, Haimin, ApJ, 946, 64

2021

1. An MHD Modeling of the Successive X2.2 and X9.3 Solar Flares of 2017 September 6 [19]
   Inoue, Satoshi & Bamba, Yumi, ApJ, 914, 71
2. Understanding the Initiation of the M2.4 Flare on 2017 July 14 [9]
   Jing, Ju, Inoue, Satoshi, Lee, Jeongwoo, Li, Qin, Nita, Gelu M., Xu, Yan, Liu, Chang, Gary, Dale E. & Wang, Haimin, ApJ, 922, 108
3. Evolution of the Nonpotential Magnetic Field in the Solar Active Region 12673 Based on a Nonlinear Force-free Modeling [13]
   Yamasaki, Daiki, Inoue, Satoshi, Nagata, Shin'ichi & Ichimoto, Kiyoshi, ApJ, 908, 132

2020

1. Intrusion of Magnetic Peninsula toward the Neighboring Opposite-polarity Region That Triggers the Largest Solar Flare in Solar Cycle 24 [12]
   Bamba, Yumi, Inoue, Satoshi & Imada, Shinsuke, ApJ, 894, 29
2. Forward Modeling of Particle Acceleration and Transport in an Individual Solar Flare [16]
   Gordovskyy, Mykola, Browning, Philippa K., Inoue, Satoshi, Kontar, Eduard P., Kusano, Kanya & Vekstein, Grigory E., ApJ, 902, 147
3. Chromospheric Magnetic Field: A Comparison of He I 10830 Å Observations with Nonlinear Force-free Field Extrapolation [12]
   Kawabata, Yusuke, Asensio Ramos, Andrés, Inoue, Satoshi & Shimizu, Toshifumi, ApJ, 898, 32
4. A Magnetohydrodynamic Relaxation Method for Non-force-free Magnetic Field in Magnetohydrostatic Equilibrium [14]
   Miyoshi, Takahiro, Kusano, Kanya & Inoue, Satoshi, ApJS, 247, 6
5. Comparative Study of Data-driven Solar Coronal Field Models Using a Flux Emergence Simulation as a Ground-truth Data Set [34]
   Toriumi, Shin, Takasao, Shinsuke, Cheung, Mark C. M., Jiang, Chaowei, Guo, Yang, Hayashi, Keiji & Inoue, Satoshi, ApJ, 890, 103
6. Serial Flaring in an Active Region: Exploring Why Only One Flare Is Eruptive [4]
   Woods, Magnus M., Inoue, Satoshi, Harra, Louise K., Matthews, Sarah A. & Kusano, Kanya, ApJ, 890, 84