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Spectral Characterisation of the Osterseen Lake District - EARSeL ...

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3 DATA<br />

Hamburg<br />

Germany<br />

Munich<br />

Berlin<br />

Lustsee Grobensee<br />

N<br />

Westl.<br />

Breitenauersee<br />

Härtlings Sill<br />

Lintensee<br />

Stechsee<br />

Ameisensee<br />

Östl. Breitenauersee<br />

Ground Water<br />

Wellspring<br />

Großer Ostersee<br />

Eishaussee<br />

Brauhaussee<br />

Herrensee<br />

Fischkaltersee<br />

Forchensee<br />

Wolfelsee<br />

Sengsee<br />

Fohnsee<br />

Schiffhüttensee<br />

Waschsee<br />

Figure 1. Location <strong>of</strong> <strong>the</strong> test area "<strong>Osterseen</strong> <strong>Lake</strong> <strong>District</strong>" south <strong>of</strong> Munich, Germany.<br />

0 500 m<br />

3.1. Hyperspectral remote sensing data acquired by ROSIS sensor<br />

The Reflective Optics System Imaging Spectroradiometer (ROSIS) was developed since 1986 in cooperation<br />

between DLR, GKSS, and MBB (now Astrium) [5][6][7]. It is a push broom scanner with 512 spatial and 115<br />

spectral pixels recording in <strong>the</strong> wavelength range between 430 nm and 860 nm. The spectral sampling interval<br />

amounts 4 nm and <strong>the</strong> full width at half maximum is about 7.5 nm. With an instantaneous field <strong>of</strong> view <strong>of</strong> 0.59<br />

mrad <strong>the</strong> spatial resolution results in 2.8 x 2.8 m² at a flight altitude <strong>of</strong> 5,000 m.<br />

The data presented in this study were recorded on June 5 th , 2001 between 10:42 and 11:20 UTC in a nor<strong>the</strong>rly flight<br />

direction at an altitude <strong>of</strong> about 5,000 m. The data were radiometrically corrected based on laboratory<br />

measurements using a calibrated light source. The geometric correction <strong>of</strong> <strong>the</strong> distortions due to flight attitude (roll,<br />

pitch, and yaw angles) uses information from <strong>the</strong> airplane's inertial system, <strong>the</strong> flight velocity, <strong>the</strong> altitude above<br />

ground, and <strong>the</strong> focal length <strong>of</strong> <strong>the</strong> telescope [8]. The radiometrically and geometrically corrected composit <strong>of</strong> two<br />

flight lines is shown in Fig. 2.<br />

447

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