pybsm.radiance.functional
The Python Based Sensor Model (pyBSM) is a collection of electro-optical camera modeling functions.
Developed by the Air Force Research Laboratory, Sensors Directorate.
Author citation: LeMaster, Daniel A.; Eismann, Michael T., “pyBSM: A Python package for modeling imaging systems”, Proc. SPIE 10204 (2017)
Distribution A. Approved for public release. Public release approval for version 0.0: 88ABW-2017-3101 Public release approval for version 0.1: 88ABW-2018-5226
Maintainer: Kitware, Inc. <nrtk@kitware.com>
This module deals with all things related to radiance, including black body spectral emission calculations, spectral atmospheric absorption, and conversion of radiance to photons. Anything material with a non-zero temperature emits electromagnetic radiation according to Planck’s law and its temperature, spectral emissivity.
Functions
Converts pupil plane radiance to focal plane irradiance for an extended source. |
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Calculates blackbody spectral radiance. |
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Check to see if the total collected photoelectrons are greater than the desired maximum well fill. |
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Represents spectral irradiance on the FPA due to emissions from the walls of the dewar itself. |
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For infrared systems, this term represents spectral irradiance emitted by the cold stop on to the FPA. |
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IBSM Equation 3-34. |
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This function provides target and background spectral radiance as defined by the GIQE. |
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This term represents spectral irradiance emitted by the optics (but not the cold stop) on to the FPA. |
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IBSM Equation 3-42 with dark current, integration time, and tdi separated out. |
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Calculates extended target contrast SNR for semiconductor-based photon detector systems. |
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Provides a mapping between reflectance on the ground and photoelectrons collected in the sensor well. |
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Resamples arrays that are input as a function of wavelength. |
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For semiconductor-based detectors, returns the signal rate generated at the output as well as other quantities. |
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Calculates total spectral radiance at the aperture for a object of interest. |