40. Fast Convective Flows Throughout the Near-Surface Shear Layer
Ring-diagram analysis reveals that the convective flow speed inside the Sun is consistent with most numerical simulations of global convection.
Monthly Archives: June 2015
39. Solar Cycle Variation of the Inter-Network Magnetic Field
Solar inter-network magnetic field, the weakest component of the solar magnetism, seems to be invariant at ~10 G from the minimum to the maximum phase of Cycle 24. This suggests a possible origin of small-scale, local dynamo.