Commentary Relative to the Emission Spectrum of the Solar Atmosphere: Further Evidence for a Distinct Solar Surface

Progress in Physics. 2013;9(3):1.2-1.3


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Journal Title: Progress in Physics

ISSN: 1555-5534 (Print); 1555-5615 (Online)

Publisher: HEXIS (Arizona)

LCC Subject Category: Science: Physics

Country of publisher: United States

Language of fulltext: English

Full-text formats available: PDF



Robitaille P.-M.


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Time From Submission to Publication: 1 weeks


Abstract | Full Text

The chromosphere and corona of the Sun represent tenuous regions which are characterized by numerous optically thin emission lines in the ultraviolet and X-ray bands. When observed from the center of the solar disk outward, these emission lines experience modest brightening as the limb is approached. The intensity of many ultraviolet and X-ray emission lines nearly doubles when observation is extended just beyond the edge of the disk. These findings indicate that the solar body is opaque in this frequency range and that an approximately two fold greater region of the solar atmosphere is being sampled outside the limb. These observations provide strong support for the presence of a distinct solar surface. Therefore, the behavior of the emission lines in this frequency range constitutes the twenty fifth line of evidence that the Sun is comprised of condensed matter