2000
DOI: 10.1016/s1350-4495(00)00039-6
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A spectral performance model for the High Resolution Dynamics Limb Sounder (6–18 μm)

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Cited by 5 publications
(2 citation statements)
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“…This model uses both the calculated and measured spectral characteristics of each optical train element to determine the integrated end-to-end spectral throughput. The results of the model demonstrate the predicted instrument level performance, from which the mean IB throughput response is determined [24] . The predicted instrument throughput was derived by combining the spectral R% or T% properties of the components along the optical train, assuming the absence of multiple beaming between elements.…”
Section: System Throughput Performancementioning
confidence: 69%
“…This model uses both the calculated and measured spectral characteristics of each optical train element to determine the integrated end-to-end spectral throughput. The results of the model demonstrate the predicted instrument level performance, from which the mean IB throughput response is determined [24] . The predicted instrument throughput was derived by combining the spectral R% or T% properties of the components along the optical train, assuming the absence of multiple beaming between elements.…”
Section: System Throughput Performancementioning
confidence: 69%
“…Astronomical spectroscopy requires precise filtering to reject undesirable spectral radiation while maximizing the throughput within the required isolated passband. 1,2 Dichroic beamsplitters, or dichroics, are filters that rely on the optical interference occurring within thin-film layers to ensure the transmission and reflection of selective wavelengths from an incident light beam. They play a vital role in determining spectral response measurements and are, thus, critical optical components for selecting and isolating wavebands for astronomical observation.…”
Section: Introductionmentioning
confidence: 99%