The challenge of this calibration development is to achieve better performance than the item under test using mostly standard items. Because only the subsystem spectrometer needs to be calibrated, the calibration facility needs to simulate the geometrical “behaviours” of the imaging system. A trade-off study indicates that no commercial devices are able to fulfil completely all the requirements so that it was necessary to opt for an in home telecentric achromatic design. The proposed concept is based on an Offner design. This allows mainly to use simple spherical mirrors and to cover the spectral range. The spectral range is covered with a monochromator. Because of the large number of parameters to record the calibration facility is fully automatized. The performances of the calibration system have been verified by analysis and experimentally. Results achieved recently on a free-form grating Offner spectrometer demonstrate the capacities of this new calibration facility. In this paper, a full calibration facility is described, developed specifically for a new free-form spectro-imager. |
I.INTRODUCTIONThe availability of free form manufacturing tools allows the development of new type of spectrometers. To be confident in these new designs and new manufacturing process, it is requested to develop metrology tools able to confirm/evaluate their performances. The basic performances are the spectral one as spectral response, resolution, and registration, but the geometrical one as MTF, the polarization and the straylight remains also important characteristics to verify. To reply to these new demands a dedicated optical ground system equipment (OGSE) has been developed at the Centre Spatial de Liège. The application case is a recently free-form grating Offner developed by AMOS[1]. This spectrometer is very compact and lightweight for an implementation on a small platform. The design offers an excellent image quality while maintaining very low spectral (smile) and spatial (keystone) distortions. The metrology system needs to have better performances than the instrument under test and needs to simulate the geometrical properties of the front imaging system. II.TRADE-OFFA.IntroductionThe guide line for the development of the test bench was to allow the full characterization of a spectrometer including a free from grating, part of a spectro-imager. The design of this spectrometer is shown in Figure 1 and is based on an original modified-Offner design for imaging spectrometer with a convex gratings ruled on a Free-Form surface [1]. This required an imaging system that shapes the input beam as the one provided by the imaging system. B.Tests to be performedImaging spectrometer main performances to be characterized are the following: Each test will be briefly described in section V. To do these characterizations, the calibration setup needs:
The full calibration facility is described in next section. C.Input light shape constraintsThe input light should be similar to the output of the coming imaging system. In this case, it will be a TMA telescope. In particular, the design of the telescope is telecentric (the variation of the chief ray incidence along the FOV can be neglected), nearly achromatic, with a F/# = 5. Moreover, it is requested to illuminate in one shot the full spectrometer entrance slit (62 mm long). D.Proposed solutionThe calibration test setup has to image an object placed at a finite distance. A trade-off study indicates that no commercial devices are able to fulfill all requirements. It was thus necessary to go to an homemade telecentric achromatic design. To be close as possible to the telescope properties at spectrometer entrance slit, the proposed concept is based on an Offner design (see Fig. 3). This design uses simple spherical mirrors. The system is achromatic, telecentric with a magnification of 1, and is designed with a F/# < 5 to fit with the imaging F/#. III.CALIBRATION TEST SET-UPA.Test setup elementsThe final design and configuration is depicted in Fig. 4 and Fig. 5. It is composed of:
The calibration facility generates a quasi-monochromatic (with tunable Δλ and λ) and uniform (thanks to the IS) illumination on the entrance slit of the spectrometer under test. For each performance test, a dedicated object target is placed at the IS output (see section III.B): it will be imaged (ratio 1:1) exactly on the spectrometer entrance slit. Each element position is adaptable (with accurate translation/rotation stages) for fine tuning alignment. B.Target objectsFor each performance test, a dedicated target object has been performed at CSL. Some pictures are depicted in Fig. 6. The targets are inserted in specific housing adapted for an accurate positioning in the mounting aligned in the calibration setup under the IS. C.Test setup fully automatizedBecause of the large number of parameters to record, the calibration facility is completely automatized. The Labview program controls:
The program manages the positions and wavelength scanning for each test configuration. Images recorded by the camera at each step are automatically classified to be analyzed. D.Setup alignmentAlignment consists mainly to co-align both mirrors (M1 and M2), and to localize exactly entrance and exit slits. For this purpose, slits are materialized by metallic spheres. A first alignment was done with an API Radian laser tracker, completed after by an interferometric alignment. This interferometric alignment uses those metallic spheres to measure the WFE across the Offner Relay. The aberrations are minimized by tuning mirrors and entrance slit positions. At the optimum configuration, all positions are fixed. Metallic spheres at the exit of the Offner Relay are then placed at the focal point of the interferometer. The WFE measurement for the final frozen configuration of the CSL Offner relay is shown in Fig. 7. Astigmatism is the main contributor to the WFE, but the RMS value is considered as sufficiently low. Once Offner relay has been aligned, the second step is to align the spectrometer: its entrance slit shall coincide with the Offner relay exit slit (materialized by metallic spheres). A first alignment has been carried out by laser tracker: positions of the exit slit metallic spheres are recorded and entrance slit of the spectrometer is placed with the X,Y,Z motorized translation stages, at that position. Then, it is the image on the spectrometer camera that is used to refine the alignment: a slit theoretically thinner than a pixel is placed at Offner relay entrance, the focus is adjusted in order to image this slit on about 1 pixel on the camera. IV.SETUP CHARACTERIZATIONB.Spatial uniformityThe setup was designed to uniformly illuminate an exit slit around 60mm long. The exit slit spatial uniformity of the Offner relay is mainly linked to the IS output. It has been measured with the set-up depicted in Fig. 8. The monochromator is working on the 0th diffraction order, illuminating the slit with a polychromatic light. An optical fiber (20 μm width) with a NA=0.1 is used in order to analyze only infield light (F/#~5, comparable to the spectrometer F/#). The fiber is connected to a photodetector, and fixed on a translation stage to scan the full exit slit. Results are presented in Fig. 9: the Offner relay reaches 99% uniformity over 59mm. C.StraylightTo measure Offner relay straylight at exit slit, for in field light, the set-up presented in Fig. 10 is used. It allows a scan of the Offner relay focal plane to investigate the transition of a knife-edge placed at the entrance slit. Measurement results are depicted in Fig. 11. Averaged straylight at 250 μm from the cut is around 0.13% ± 0.01% D.IrradianceIrradiance at spectrometer entrance slit (F/#5 field) has been measured with a calibrated photodiode, depicted in Fig. 12. Even if the irradiance is small, for the tested spectrometer, enough flux is collected by the camera in its focal plane to achieve good S/N image. E.PolarizationTo test polarization sensitivity, the input light has to be nearly non-polarized. Offner relay output light polarization has thus been measured. The set-up is depicted in Fig. 13, using a linear motorized rotating polarizer to scan polarization angles. Measurements are influenced by two main factors: Since the Offner relay polarization is known (Fig. 14 and Fig. 15) it can be removed, and by this way the tested spectrometer (including camera) polarization behaviour is known with an accuracy of 0.5%. V.TESTS DESCRIPTIONA.KeystoneThe Keystone is defined as the departure from straightness and parallelism of line spectra from white point sources at various positions in the image field. For this test:
B.Spectral response matrixThis characterization includes spectral range, spectral resolution, peak transmission, smile and tilt, and out-of-band rejection. The goal is to build a 3D spectral response matrix. All this information can be extracted from a spectral scan (Δλ =2.5 nm, for λ =400 to 950 nm) performed by the monochromator. For this configuration, no slit in object plane is needed: a full line along geometrical dimension will be registered at different spectral positions according to λ. C.MTFTwo kind of MTF can be measured: in spatial direction, or in spectral direction. MTF is extracted from LSF. To do LSF measurement, there are two configurations:
D.Polarization sensitivityPolarization sensitivity measurement implies image registration according incident light polarization angle. For this purpose, a motorized rotating polarizer is placed in front of the spectrometer entrance slit. By removing the polarizer artifact and previously characterized Offner polarization signature (see section IV.E), the spectrometer polarization sensitivity can be extracted. This measurement can be done with polychromatic light or quasi-monochromatic light. E.StraylightIn-field straylight is measured by placing a knife-edge in the object plane of the calibration setup in order to mask half of the image plane surface (along spatial direction), see central picture of Fig. 6. Images have been recorded for different wavelengths (Δλ ~10nm) and for white light (example in the second picture of Fig. 16). Removing background, these images gives information on straylight with respect to the distance from the knife-edge. VI.CALIBRATION CAMPAIN RESULTS EXAMPLESThis calibration facility was prepared and used to calibrate a new free-form compact spectro-imager. Some captured images are depicted in Fig. 16. Detailed analysis of performances, including their extraction methodology from measurement, can be found in Ref. [1]. VII.CONCLUSIONNew types of spectrometers for Earth observation are under development, modifying requirement for calibration facilities. Their designs become then more challenging. In this paper, design and performances of a new calibration facility for spectro-imager has been presented. The developed calibration facility was certified fully compliant to characterize the new spectro-imager presented in Ref [1]. Collaboration will continue for the next spectrometer generation, which will be tested with the same calibration setup. An adaptation of this calibration setup will also be developed to perform calibration in vacuum environment. VIII.ACKNOWLEDGEMENTThis development would not have been possible without the financial support of the Belgian Space Officethrough the ESA GSTP program. IX.IX.REFERENCESV. Moreau, J. Versluys, M. François, M. Taccola, C. Michel, P. Blain, and Y. Stockman,
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