| huangshan |
2008-08-12 11:26 |
Summary ue/GB+U
This study is a detailed follow-up to two previous studies concerning stray light in the EO-1 +CQ$-3
telescope (see EO-1 Stray Light Analysis Reports 1 and 2). Following coating of the EO-1 flight cD!y d^QE
mirrors, the BRDF was measured by SSG, then re-measured by Schmitt Measurement Systems. @/DHfs 4O
The stray spectral radiance from the Stray Radiation Scene described in the LANDSAT 7 .5ItH^
specification was recalculated using the Schmitt BRDF measurements and a simple spreadsheet 4ne95_i
calculation. This calculation assumes the Point Source Transmittance (PST) is rotationally
n}f*>Mn
symmetric, and does an integration over the Stray Radiation Scene. q ad`muAd
To refine this estimate of stray radiance, ray-trace simulations were done using TracePro to better AVR=\ qR
predict the PST. The PST was used to calculate the stray spectral radiance using a C++ computer #&oL iz=hZ
program written for this purpose. The stray spectral radiance was computed by integrating over CSBk
the LANDSAT 7 Stray Radiation Scene, weighed by the PST.
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