297 citations · 412 across the 7 of their papers we have counts for
7 papers
Eruptivity of Flaring Active Regions Based on Electric Current Neutralization and Torus Instability Analysis
Johan Muhamad, Kanya Kusano
Solar flares are frequently accompanied by coronal mass ejections (CMEs) that release significant amount of energetic plasma into interplanetary space, potentially causing geomagne…
Convective Magnetic Flux Emergence Simulations from the Deep Solar Interior to the Photosphere: Comprehensive Study of Flux Tube Twist
Shin Toriumi, Hideyuki Hotta, Kanya Kusano
The emergence of magnetic flux from the deep convection zone plays an important role in the solar magnetism, such as the generation of active regions and triggering of various erup…
Data-driven MHD Simulation of the Formation of a Magnetic Flux Rope and an Inclined Solar Eruption
Yeongmin Kang, Takafumi Kaneko, K. D. Leka +1
Solar energetic events are caused by the release of magnetic energy accumulated in the solar atmosphere. To understand their initiating physical mechanisms, the dynamics of the cor…
Double arc instability in the solar corona
N. Ishiguro, K. Kusano
The stability of the magnetic field in the solar corona is important for understanding the causes of solar eruptions. Although various scenarios have been suggested to date, the te…
Simulation Study of Hemispheric Phase-Asymmetry in the Solar Cycle
D. Syukuya, K. Kusano
Observations of the sun suggest that solar activities systematically create north-south hemispheric asymmetries. For instance, the hemisphere in which the sunspot activity is more…
Structure and Stability of Magnetic Fields in Solar Active Region12192 Based on Nonlinear Force-Free Field Modeling
S. Inoue, K. Hayashi, K. Kusano
We analyze a three-dimensional (3D) magnetic structure and its stability in large solar active region(AR) 12192, using the 3D coronal magnetic field constructed under a nonlinear f…
Super-Droplet Method for the Numerical Simulation of Clouds and Precipitation: a Particle-Based Microphysics Model Coupled with Non-hydrostatic Model
Shin-ichiro Shima, Kanya Kusano, Akio Kawano +2
A novel, particle based, probabilistic approach for the simulation of cloud microphysics is proposed, which is named the Super-Droplet Method (SDM). This method enables accurate si…