SCHOTT optical glass in space

Ralf Jedamzik; Uwe Petzold

doi:10.1117/12.2272714

5 September 2017 SCHOTT optical glass in space

Ralf Jedamzik, Uwe Petzold

Proceedings Volume 10401, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems; 104010I (2017) https://doi.org/10.1117/12.2272714
Event: SPIE Optical Engineering + Applications, 2017, San Diego, California, United States

Abstract

Optical systems in space environment have to withstand harsh radiation. Radiation in space usually comes from three main sources: the Van Allen radiation belts (mainly electrons and protons); solar proton events and solar energetic particles (heavier ions); and galactic cosmic rays (gamma- or x-rays). Other heavy environmental effects include short wavelength radiation (UV) and extreme temperatures (cold and hot). Radiation can damage optical glasses and effect their optical properties. The most common effect is solarization, the decrease in transmittance by radiation. This effect can be observed for UV radiation and for gamma or electron radiation. Optical glasses can be stabilized against many radiation effects. SCHOTT offers radiation resistant glasses that do not show solarization effects for gamma or electron radiation. A review of SCHOTT optical glasses in space missions shows, that not only radiation resistant glasses are used in the optical designs, but also standard optical glasses. This publication finishes with a selection of space missions using SCHOTT optical glass over the last decades.

Citation Download Citation

Ralf Jedamzik and Uwe Petzold "SCHOTT optical glass in space", Proc. SPIE 10401, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems, 104010I (5 September 2017); https://doi.org/10.1117/12.2272714

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