Large-Scale Solar Magnetic Fields Observed with the Infrared
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Variations in Ratio and Correlation of Solar Magnetic Fields in
On the Differences in the Ambient Solar Wind Speed Forecasting
X. F. Wang's research works Chinese Academy of Sciences, Beijing
Regions of coronal holes on the solar surface (calculated in the
Panel (a): Magnetogram in the blue wing of the spectral line
Variations in Ratio and Correlation of Solar Magnetic Fields in
X. F. Wang's research works Chinese Academy of Sciences, Beijing
Analytic representation of the red V /I line ratio in units of the
Screenshot of the display on a computer screen when downloading
PDF) Spatially resolved measurement of helium atom emission line
Large-Scale Solar Magnetic Fields Observed with the Infrared
Comparison between the 31 August 2017 HMI and STOP magnetograms
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