Research interests of KNAG includes numerical astrophysics of
| Date/Time | Presentation |
|---|---|
| September 14 (Friday), 3pm | Kang, Hyesung - Problems in Estimating Non-thermal Radiation from Supernova Remnants |
| Cho, Jungyeon - Growth of a Localized Seed Magnetic Field in Turbulence | |
| Guo, Zhibin - Heat Transport in Tangled Magnetic Fields | |
| October 5 (Friday), 3pm | Ko, Juyeon - Distribution Analysis of Density, Temperature, and Velocity Field around the Clusters |
| Hong, Sungwook - Strong Accretion Shock Waves in Cluster Outskirts and Possibility of Cosmic Ray Population Inversion | |
| Ahn, Kyungjin - Current Status of 21CMA | |
| Ryu, Dongsu - Cosmic Magnetism | |
| October 26 (Friday), 3pm | Jang, Hanbyul - A Relativistic MHD Code based on an Upwind Scheme |
| Seo, Woo-Young - Numerical Simulations of Star Formation in Barred Galaxies | |
| Yoo, Hyunju - Effect of Forcing Scale on MHD Turbulence | |
| November 16 (Friday), 3pm | Kim, Yonghwi - |
| Yoon, Heesun - | |
| Hong, Sungwook - | |
| Kwak, Kyujin - |
| Date/Time | Presentation |
|---|---|
| November 25 (Friday), 3pm | Kwon, Hyewon - Study of Astrophysical Shock Waves using a PIC Code |
| Seo, Wooyoung - Star Formation Feedback in Barred Galaxies | |
| Kim, Hoonkyu - Inverse Energy Cascade and Magnetic Helicity in 3D Driven Electron MHD (EMHD) Turbulence | |
| Akahori, Takuya - Shock and Turbulence in Galaxy Clusters and the Large-Scale Structure | |
| November 4 (Friday), 3pm | Jang, Hanbyul - Toward a Relativistic Magnetohydrodynamic Code |
| Kim, Jeong-Gyu - Gravitational Instability in Vertically Stratified/Pressure-confined Disks | |
| Yoo, Hyunju - Effects of Multiple Driving Scales on Turbulence Statistics | |
| Yoon, Heesun - Estimate the Magnetic Field Strength using Rotation Measure | |
| October 14 (Friday), 3pm | Kim, JiHee - Updated Comparison study of Extensive Air Shower Simulations with CORSIKA and COSMOS |
| Kim, Yonghwi - Effects of Spiral Arms on the Gaseous Features of Barred Spiral Galaxies | |
| Cho, Hyunjin - Probability Distribution Function of Density in Turbulent Molecular Clouds | |
| Ahn, Kyungjin - Probing the First Stars through Planck | |
| September 23 (Friday), 3pm | Roh, Soonyoung - A Comparative Study of COSMOS and CORSIKA Extensive Air Shower Simulations |
| Park, Junseung - A Scaling of Velocity and Magnetic Fields in Decaying Turbulence in Expanding/Collapsing Media | |
| Hong, Sungwook - 2D Genus Topology of 21cm Differential Brightness Temperature during Cosmic Reionizationi | |
| Ryu, Dongsu - Magnetic Field in Voids |
| Date/Time | Presentation |
|---|---|
| December 17 (Friday), 3pm | Jang, Hanbyul - Relativistic Hydrodynamic Code for Multi-component Fluids |
| Yoon, Hee-Sun - Correlation between Density and Magnetic Field Strengths in Compressible MHD Turbulence | |
| Yoo, Hyun-Ju - Statistics of Isothermal Compressible Turbulence in Simulations: Single versus Double Forcing | |
| Kim, Jongsoo - Introduction to CUDA Programming Basics | |
| November 26 (Friday), 3pm | Kim, Jeong-Gyu - Gravitational Instability of Pressure-confined Rotating Polytropic Disks |
| Kim, Hoon-Kyoo - Inverse Energy Cascade of Semi-2D Turbulence | |
| Ahn, Kyungjin - Cosmic Reionization by the First Stars | |
| Cho, Jungyeon - Non-locality of HD and MHD Turbulence | |
| October 22 (Friday), 3pm | Park, Junseung - MHD Turbulence in Expanding/Collapsing Media |
| Cho, Hyunjin - Turbulence in Molecular Clouds: Observation versus Simulation | |
| Akahori, Takuya - Exploring Faraday Rotation Measure due to the Intergalactic Magnetic Field with the Square Kilometer Array | |
| Kang, Hyesung - Cosmic Ray Spectrum in SN Ia Remnants | |
| September 10 (Friday), 3pm | Kim, Chang-Goo - Regulation of Star Formation Rates in Multiphase Galactic Disks: Numerical Tests of the Thermal/Dynamical Equilibrium Model |
| Roh, Soonyoung - Dethinning Algorithm in Air Shower Simulations | |
| Kim, JiHee - Energy Estimator of Ultra-High Energy Cosmic Rays(UHECRs) Using GEANT4 Simulation | |
| Ryu, Dongsu - A Model for the Intergalactic Magnetic Field and its Astrophysical Implications |