212. Deconvolving SDO/HMI Intensity and Vector Magnetic Field Data to Achieve Hinode/SOT-SP Quality
211. Electric Current Neutralization and Critical Height of Flux Rope in Eruptive and Non-Eruptive Active Regions
210. The Role of Electric Currents in the October 2014 X1.6 Solar Flare
209. The Magnetic Origin of Chromospheric Moreton Waves
208. Unveiling Key Factors in Solar Eruptions Leading to the Solar Superstorm in May 2024
207. Simulating the formation and eruption of magnetic flux ropes in the solar atmosphere
206. Magnetic power spectra of the Sun and cycle dependence of magnetic network
205. Is the solar meridional circulation profile single-, double-, or multiple-cell?
204. Exploring Meridional Flow in the Solar Polar Caps
A surface flux transport model, using HMI-observed global magnetic field and active regions as inputs, with different polar meridional-flow profiles simulates the magnetic field in the polar caps. The simulation is then compared with Hinode-observed polar magnetic fields. The result supports an existence of counter cells above 70-degree latitude in each hemisphere.