Large-Scale Solar Magnetic Fields Observed with the Infrared

On the Differences in the Ambient Solar Wind Speed Forecasting

Different ways to represent the magnetograms, obtained

Spatially resolved measurement of helium atom emission line

Angular Dependence of the Facular–Sunspot Coverage Relation as

WSO (top panel), STOP (middle panel), and IRmag (bottom panel

Near-infrared Stokes spectropolarimetry of fusion-related toroidal

Large-Scale Solar Magnetic Fields Observed with the Infrared

Different ways to represent the magnetograms, obtained

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

Large-Scale Solar Magnetic Fields Observed with the Infrared

Same as in Figure 1, but a SMAT magnetogram obtained with a

Panel (a): Comparison between the observed (points) Stokes

PDF) Calibration of the 6302/6301 Stokes V line ratio in terms of