Summary v4zd
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This study is a detailed follow-up to two previous studies concerning stray light in the EO-1 u9gr@06
telescope (see EO-1 Stray Light Analysis Reports 1 and 2). Following coating of the EO-1 flight 5->PDp
mirrors, the BRDF was measured by SSG, then re-measured by Schmitt Measurement Systems. ;?o C=c
The stray spectral radiance from the Stray Radiation Scene described in the LANDSAT 7 f!J^vDl
specification was recalculated using the Schmitt BRDF measurements and a simple spreadsheet ~JNuy"8
calculation. This calculation assumes the Point Source Transmittance (PST) is rotationally $K KaA{ 0-
symmetric, and does an integration over the Stray Radiation Scene. ,pASjFWi
To refine this estimate of stray radiance, ray-trace simulations were done using TracePro to better CbH Nb~
predict the PST. The PST was used to calculate the stray spectral radiance using a C++ computer P8VU&b\
program written for this purpose. The stray spectral radiance was computed by integrating over Qm.kXlsDI
the LANDSAT 7 Stray Radiation Scene, weighed by the PST.
