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NASA NTRS · 19730048326

A biased model for calculating the evolution in solar absorptance.

Abstract

A biased model is proposed to account for the smooth curve type of degradation experienced by spacecraft environmental interfacing materials. Because the space environment is nondestructive, the solar absorptance (alpha) must reach its maximum value in finite time, monotonically, without inflection points and be single valued, viz., alpha equals alpha-zero plus (Bt - D) exp (-At). A simple procedure is also included for the parametric calculation of A, B, and D with respect to solar intensity, particle flux, and temperature. The suitability of the model is discussed with regard to destructive testing, and a more general equation proposed. Use of the model for alpha calculations appropriate to the HELIOS missions is outlined.

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BibTeXRIS

Schutt, J. B., Duncan, C. H.. 1973-01-01. A biased model for calculating the evolution in solar absorptance.. https://ntrs.nasa.gov/citations/19730048326

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