Synthetic DKIST/DL-NIRSP observations of the quiet Sun show that standard inversion plus flow tracking recovers only about 50 to 70 percent of the unsigned Poynting flux and badly underestimates the net flux, mostly through missing horizontal shearing motions.
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What Can DKIST/DL-NIRSP Tell Us About Quiet-Sun Magnetism?
Synthetic DKIST/DL-NIRSP observations of the quiet Sun show that standard inversion plus flow tracking recovers only about 50 to 70 percent of the unsigned Poynting flux and badly underestimates the net flux, mostly through missing horizontal shearing motions.