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NASA NTRS · 19700000372

Heat-rejection windows for telescopes

Abstract

Heat-rejection telescope windows reflect incident solar energy outside the hydrogen-alpha line while processing a peak transmission exceeding fifty percent at 6563 angstrom units. The windows also function as secondary blocking filters to the telescope's Fabry-Perot filter.

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BibTeXRIS

Austin, R., Rehnberg, J.. 1970-09-01. Heat-rejection windows for telescopes. https://ntrs.nasa.gov/citations/19700000372

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