Publications of Takafumi Kaneko

A list of publications authored or co-authored by Takafumi Kaneko, 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: 0000-0002-7800-9262

List of publications ordered by citations
Number of papers: 10 (refereed: 10)
No. of citations: 189
First author papers: 7 (refereed: 7)

2025

1. Conditions for Solar Prominence Formation Triggered by Single Localized Heating [8]
   Yoshihisa, Takero, Yokoyama, Takaaki & Kaneko, Takafumi, ApJ, 978, 94

2024

1. Data-driven MHD Simulation of the Formation of a Magnetic Flux Rope and an Inclined Solar Eruption [2]
   Kang, Yeongmin, Kaneko, Takafumi, Leka, K. D. & Kusano, Kanya, ApJ, 974, 168

2023

1. Characteristics of the Accelerated Electrons Moving along the Loop Derived from Cyclical Microwave Brightenings at the Footpoints [1]
   Matsumoto, Keitarou, Masuda, Satoshi & Kaneko, Takafumi, ApJ, 955, L39

2022

1. Impact of subsurface convective flows on the formation of sunspot magnetic field and energy build-up [8]
   Kaneko, Takafumi, Hotta, Hideyuki, Toriumi, Shin & Kusano, Kanya, MNRAS, 517, 2775

2021

1. Data-driven MHD Simulation of Successive Solar Plasma Eruptions [24]
   Kaneko, Takafumi, Park, Sung-Hong & Kusano, Kanya, ApJ, 909, 155

2018

1. Impact of Dynamic State on the Mass Condensation Rate of Solar Prominences [22]
   Kaneko, Takafumi & Yokoyama, Takaaki, ApJ, 869, 136

2017

1. Reconnection-Condensation Model for Solar Prominence Formation [54]
   Kaneko, Takafumi & Yokoyama, Takaaki, ApJ, 845, 12

2015

1. Apparent Cross-field Superslow Propagation of Magnetohydrodynamic Waves in Solar Plasmas [24]
   Kaneko, T., Goossens, M., Soler, R., Terradas, J., Van Doorsselaere, T., Yokoyama, T. & Wright, A. N., ApJ, 812, 121
2. Numerical Study on In-Situ Prominence Formation by Radiative Condensation in the Solar Corona [37]
   Kaneko, T. & Yokoyama, T., ApJ, 806, 115

2014

1. Simulation Study of Solar Plasma Eruptions Caused by Interactions between Emerging Flux and Coronal Arcade Fields [9]
   Kaneko, Takafumi & Yokoyama, Takaaki, ApJ, 796, 44