New earth system model for optical performance evaluation of space instruments

Dongok Ryu, Sug Whan Kim, Robert P. Breault

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)

Abstract

In this study, a new global earth system model is introduced for evaluating the optical performance of space instruments. Simultaneous imaging and spectroscopic results are provided using this global earth system model with fully resolved spatial, spectral, and temporal coverage of sub-models of the Earth. The sun sub-model is a Lambertian scattering sphere with a 6-h scale and 295 lines of solar spectral irradiance. The atmospheric sub-model has a 15-layer three-dimensional (3D) ellipsoid structure. The land sub-model uses spectral bidirectional reflectance distribution functions (BRDF) defined by a semi-empirical parametric kernel model. The ocean is modeled with the ocean spectral albedo after subtracting the total integrated scattering of the sun-glint scatter model. A hypothetical two-mirror Cassegrain telescope with a 300-mm-diameter aperture and 21.504 mm x 21.504-mm focal plane imaging instrument is designed. The simulated image results are compared with observational data from HRI-VIS measurements during the EPOXI mission for approximately 24 h from UTC Mar. 18, 2008. Next, the defocus mapping result and edge spread function (ESF) measuring result show that the distance between the primary and secondary mirror increases by 55.498 μm from the diffraction-limited condition. The shift of the focal plane is determined to be 5.813 mm shorter than that of the defocused focal plane, and this result is confirmed through the estimation of point spread function (PSF) measurements. This study shows that the earth system model combined with an instrument model is a powerful tool that can greatly help the development phase of instrument missions.

Original languageEnglish
Pages (from-to)4926-4944
Number of pages19
JournalOptics Express
Volume25
Issue number5
DOIs
Publication statusPublished - 2017

Bibliographical note

Funding Information:
Center for Galaxy Evolution Research by the National Research Foundation of Korea (Grant No. 2010-0027910); Korea Astronomy and Space Science Institute (KASI) under the RandD program supervised by the Ministry of Science, ICT and Future Planning (Grant No. 2017-1-840-03). The authors would like to acknowledge the support of the Breault Research Organization through user licenses for the Advanced System Analysis Program (ASAP?) used for raytracing computations.

All Science Journal Classification (ASJC) codes

  • Atomic and Molecular Physics, and Optics

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