Comparison of Line-of-Sight Magnetograms Taken by the Solar Dynamics Observatory/Helioseismic and Magnetic Imager and Solar and Heliospheric Observatory/Michelson Doppler Imager

By Yang Liu, J. Todd Hoeksema, Philip H. Scherrer, J. Schou, S. Couvidat, R. Bush, T. Duvall, K. Hayashi, Xudong Sun, Xuepu Zhao. 2012

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Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, methodology): “…from multiple instruments, including the instruments considered in this study (see Jones & Ceja 2001; Wenzler et al. 2004, 2006; Ball et al. 2012; Liu et al. 2012) The idea is to first sort the magnetogram signal in a given magnetogram in order of strength, bin the points into N bins of equal…”
A SYSTEMATIC SURVEY OF HIGH-TEMPERATURE EMISSION IN SOLAR ACTIVE REGIONS (2012, background): “The values for the total unsigned magnetic flux we find here are similar to those from our earlier study, which used magnetogram data from the Michelson Doppler Imager (MDI) instrument onSoHO (Scherrer et al. 1995).”