Large-Scale Solar Magnetic Fields Observed with the Infrared

Spatially resolved measurement of helium atom emission line

Angular Dependence of the Facular–Sunspot Coverage Relation as

Observational results of SMAT (30 August 2017) in the red (panel

Large-Scale Solar Magnetic Fields Observed with the Infrared

Mikhail DEMIDOV, Deputy Director

Angular Dependence of the Facular–Sunspot Coverage Relation as

Panel (a): Magnetogram in the blue wing of the spectral line

X. F. Wang's research works Chinese Academy of Sciences, Beijing

On the Differences in the Ambient Solar Wind Speed Forecasting

Yoichiro HANAOKA, Doctor of Philosophy