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: 15 (refereed: 15)
No. of citations: 135
First author papers: 3 (refereed: 3)

2025

1. Data-constrained Magnetohydrodynamic Simulation for Magnetic Flux Rope Eruptions Driven by Magnetic Reconnection [0]
   Liu, Nian, Inoue, Satoshi, Wang, Ying & Wang, Haimin, ApJ, 983, 38

2024

1. Magnetic Eruption from a Three-ribbon Flare [1]
   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 [3]
   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 [8]
   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 [9]
   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 [1]
   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 [16]
   Inoue, Satoshi & Bamba, Yumi, ApJ, 914, 71
2. Understanding the Initiation of the M2.4 Flare on 2017 July 14 [8]
   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 [11]
   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 [10]
   Bamba, Yumi, Inoue, Satoshi & Imada, Shinsuke, ApJ, 894, 29
2. Forward Modeling of Particle Acceleration and Transport in an Individual Solar Flare [13]
   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 [8]
   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 [11]
   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 [32]
   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