학술논문

Impact of Film Thickness on the Spectroscopic Evolution of Polyimides in a Simulated GEO Environment
Document Type
Periodical
Source
IEEE Transactions on Plasma Science IEEE Trans. Plasma Sci. Plasma Science, IEEE Transactions on. 50(4):959-964 Apr, 2022
Subject
Engineered Materials, Dielectrics and Plasmas
Fields, Waves and Electromagnetics
Space vehicles
Image color analysis
Chemicals
Electron optics
Sea measurements
Optical variables measurement
Optical imaging
Aging
degradation
polymer films
Language
ISSN
0093-3813
1939-9375
Abstract
Space domain awareness (SDA) is becoming more important with a constantly increasing number of artificial objects in space. Astronomical reflectance spectroscopy (ARS) is a promising technique employed for remote characterization of space objects. In geosynchronous earth orbit (GEO), the chemical characteristics of a material change continuously, as it is exposed to the harsh radiation environment of several damaging species (with electrons being the primary damaging species in terms of energy deposition). These chemical modifications alter the light absorbed by and reflected from the object at certain wavelengths, resulting in a concomitant change of the measured object’s brightness and color index. By understanding the evolution of the color index of a material as a function of time on orbit, ARS can become a powerful tool for remote characterization of space objects as well as anomaly characterization and resolution. In this study, we investigate the effect of a space-simulated environment represented by high-energy (100 keV) electrons on the evolution of optical properties of several spacecraft-relevant polymer materials.