Abstract

Abstract. Hyperspectral instruments are designed for the characterisation of planetary surfaces, oceans and the atmosphere. At the moment there are a number of aircraft systems and planned space missions. Examples for this are the hyperspectral missions for Earth remote sensing (EnMAP) and also for deep space and planetary missions (Mercury mission Bepi Colombo).There are basically two options for a hyperspectral system: Snapshot systems and scanning systems. This paper investigates a scanning hyperspectral push-broom systems. In most systems the input aperture is a long slit whose image is dispersed across a 2-D detector array, so that all points along a line in the scene are sampled simultaneously. To fill out the spatial dimension orthogonal to the slit, the scene is scanned across the entrance aperture. An ideal low cost hyperspectral scanning device analogue to push broom scanner is a 2D-detector with variable spectral filters, each filter being arranged perpendicular to the direction of flight.The biggest challenge is the mapping of the images of the individual spectral channels to each other (co-registration). The solution of the problem is the prerequisite for the use of this kind of hyperspectral cameras e.g. on board of an aircraft. Therefore, an investigation should focus on the procedure of data acquisition, correction and registration. In addition, an example showing the advantages of a possible application is explained.

Highlights

  • High resolution imaging spectrometry or hyperspectral imaging (HSI) requires sophisticated solutions both for the detector and its operation as well as for the hardware and mechanics

  • An important characteristic for the spectral resolution of a camera system besides its number of spectral channels is the full width at half maximum (FWHM) of each of its bands

  • A reference channel is chosen while for the rest a Figure 10 shows the final stitched and aligned full 360◦ hyperspectral cylindrical panorama with three chosen spectral channels which where merged to RGB from a roof of German Aerospace Center (DLR) in Berlin

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Summary

Introduction

High resolution imaging spectrometry or hyperspectral imaging (HSI) requires sophisticated solutions both for the detector and its operation as well as for the hardware and mechanics. The spectrograph with grating or prism is expensive. Detector and grating ensure that the hyperspectral imager can only operate over a limited spectral range (e.g. VIS/NIR or SWIR). Alternative approaches are optical band pass filter. An important characteristic for the spectral resolution of a camera system besides its number of spectral channels is the full width at half maximum (FWHM) of each of its bands. Multispectral camera systems capture images with only a few broad bands with a few hundred nm. Hyperspectral systems, on the other hand reach a much higher spectral resolution through many narrow bands (100-200 bands with a FWHM of 5-10 nm)

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