Observational Selection Effects in Electromagnetic Wave Detection: A New Theoretical Interpretation of Solar Corona and Sunspots

We propose a novel theoretical framework suggesting that conventional electromagnetic detection systems exhibit wavelength, electromagnetic wave velocity, and angular-dependent sensitivity selection effects, which may fundamentally influence our understanding of solar corona heating mechanisms and sunspot formation. We postulate that detectors have selective sensitivity to electromagnetic waves of specific velocities, leading to observational results that may not fully reflect the true physical state of the Sun. Based on this hypothesis, we provide a unified explosive dynamics interpretation for corona hightemperature phenomena and sunspot formation, and discuss the implications of this theory for the relativistic assumption of light speed constancy.