Synthetic observations of simulated sunspot penumbrae show that spatial smearing and instrumental noise hide most opposite-polarity magnetic field patches and downflows, while overestimating their association.
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Opposite polarity magnetic field and convective downflows in a simulated sunspot penumbra
Synthetic observations of simulated sunspot penumbrae show that spatial smearing and instrumental noise hide most opposite-polarity magnetic field patches and downflows, while overestimating their association.