IJFPS · Final journal article

Sunspots, Solar Rain, Solar Prominences, Solar Tsunamis, ‎and Sunquakes as Strong Evidence for the Condensed-Matter ‎Nature of the Sun

Author(s): Jamal S. Shrair
Journal: International Journal of Fundamental Physical Sciences Year: 2026 Volume: 16 Issue: 3 Pages: 92-110 ISSN: 2231-8186

Abstract

Almost all observations discussed in this work are interpreted as supporting the condensed-matter nature of the Sun. ‎Regrettably, empirical solar data are generally interpreted with the Standard Solar Model (SSM) in mind. Consequently, ‎interpretations of solar features and phenomena are expected to remain compatible with the SSM. For instance, sunspots, ‎granules, and faculae are commonly treated as structures within a gaseous plasma, whereas the present work argues that they ‎are real physical structures formed by condensed crystal lattices. In addition, the Sun's average density (approximately 1.41 ‎g/cm³), which is comparable to that of Earth's oceans and slightly greater than that of water, is often interpreted within a ‎mathematical model rather than considered as possible evidence for a condensed state. The present work argues that the ‎overall density of the Sun is compatible with a condensed liquid state and that a purely gaseous body would not inherently ‎possess the structural properties required for the observed solar dynamo. Moreover, the continuous solar spectrum is ‎examined in relation to the physical state of solar matter. Dense, opaque matter can produce a continuous spectrum ‎approximating blackbody radiation, whereas isolated low-density gases or plasmas characteristically produce discrete ‎emission lines. Most importantly, this work argues that observed solar-dynamic phenomena such as sunspots, solar ‎prominences, coronal rain, sunquakes, and solar tsunamis cannot be adequately explained without a liquid surface and a ‎solid core.‎

Keywords

Condensed-matter SunSunspotsSolar prominencesCoronal rainSolar tsunamis
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