Table 1
Two OSIRIS NAC data sets used for the spectrophotometric analysis.
Date | UT | Distance* [km] | Scale [m/px] | Phase angle [°] | Filter no. | Filter name | Wavelength [nm] |
|
|||||||
2014-09-19 | 13.42.48 | 28.29 | 0.50 | 68.82 | 22 | Orange | 649.2 |
2014-09-19 | 13.43.00 | 28.29 | 0.50 | 68.82 | 16 | Near-UV | 360.0 |
2014-09-19 | 13.43.16 | 28.29 | 0.50 | 68.82 | 23 | Green | 535.7 |
2014-09-19 | 13.43.28 | 28.29 | 0.50 | 68.82 | 24 | Blue | 480.7 |
2014-09-19 | 13.43.40 | 28.29 | 0.50 | 68.82 | 41 | Near-IR | 882.1 |
|
|||||||
2014-09-22 | 15.49.36 | 28.40 | 0.50 | 72.03 | 22 | Orange | 649.2 |
2014-09-22 | 15.49.48 | 28.40 | 0.50 | 72.03 | 16 | Near-UV | 360.0 |
2014-09-22 | 15.50.04 | 28.40 | 0.50 | 72.04 | 23 | Green | 535.7 |
2014-09-22 | 15.50.16 | 28.40 | 0.50 | 72.04 | 24 | Blue | 480.7 |
2014-09-22 | 15.50.28 | 28.40 | 0.50 | 72.04 | 41 | Near-IR | 882.1 |
Notes. The two reference images for the image registration are indicated in bold. The same two images have been used to prepare and validate the morphological map and the boulder distributions. The first NAC set (September 19) was taken when Rosetta was at 3.33 AU from the Sun, while for the second set (September 22) the distance of the spacecraft to the Sun was 3.31 AU.
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