Performance analysis of the proposed new restoring camera for hyperspectral imaging

FFI-Report 2010

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2010/02383

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Gudrun Høye Andrei Fridman
This report investigates the performance of the proposed new restoring camera for hyperspectral imaging. The suggested camera will eliminate keystone in the postprocessing of the data with no resolution loss and will be able to collect several times more light than current hyperspectral cameras with hardware corrected keystone. A virtual camera is created in Matlab for the analyses, and data from a real hyperspectral image is used as input. The performance of the restoring camera is compared to the conventional hyperspectral cameras, that either correct keystone in hardware or apply resampling to the collected data. The analyses show that the restoring camera outperforms by far the conventional cameras under all light conditions. Conventional cameras have misregistration errors as large as 15-20%, and these errors remain even if the amount of light increases. The restoring camera, on the other hand, has negligible misregistration errors and is limited only by photon noise. This camera therefore performs better and better as the amount of light increases. In very bright light, the standard deviation of the error for the restoring camera (compared to an ideal camera) is only 0.6% and the maximum error less than 2%. The optical design for the restoring camera is included in the report. The optics is as sharp as the best conventional designs and collects four times more light. The camera must be calibrated very precisely and a method for doing so is described in the report. We have also looked briefly into the potential of resampling cameras. Resampling cameras are generally believed to be significantly worse than cameras with hardware corrected keystone. However, our analyses show that resampling cameras can compete quite well with such cameras. In particular, a resampling camera that uses a high-resolution sensor combined with binning of pixels is shown to make an excellent camera for low light applications. The performance will, however, still be noticeably worse than what can be achieved with the suggested restoring camera. We propose a joint FFI-NEO project with the goal of building the new restoring camera. The project would benefit from NEO’s expertise in design of hyperspectral cameras and FFI’s expertise in processing of hyperspectral data. Key issues to be addressed would be verification of the performance of the mixing chambers, and development and implementation of the calibration method for the camera. The outcome of the project would be a rather impressive instrument which will by far outperform the current generation of hyperspectral cameras.

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