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We develop a technique. for the analysis of He I 1083 nm spectra which addresses several difficulties through determination of a continuum background by comparison with a well calibrated standard and through removal of nearby solar and telluric blends by differential comparissri to an average spectrum. The method is compared with earlier analysis of imaging >spectroscopy obtained at the National Solar Okrvatory/Kitt Peak Vacuum Telescope (NSO/KPVT) with the NASA/NSO SpectromagnetGgraph (SPM).doi:10.1023/b:sola.0000036873.75777.33 fatcat:ehs27xphlndvpjwhaat2q7no4u