Table 1
Observing conditions for the OSIRIS images as reported in Fig. 2, where the ice spots have been identified.
N. | Time reference | Filters | d | Region | α | Δ | R | Lat | Long |
(m) | (°) | (km) | (m/px) | (°) | (°) | ||||
|
|||||||||
1 | 2015-06-27T13h26 | F22,F23,F41,F24,F71,F27,F51, | 36 | Imhotep | 89.50 | 191.94 | 3.6 | −5.8 | 189.4 |
F61,F28,F15 | |||||||||
2 | 2015-06-27T17h48 | F22,F23,F41,F24,F71,F27,F51, | 45 | Anhur | 89.39 | 188.43 | 3.5 | −41.7 | 63.7 |
F61,F28,F15 | |||||||||
3 | 2015-04-12T21h42 | F22,F23,F41,F24,F71,F27,F51 | 11 | Khonsu | 80.46 | 147.98 | 2.7 | −23.8 | 198.3 |
F61,F28,F16,F15 | |||||||||
4 | 2014-11-22T04h57 | F22,F23,F24,F27,F28,F51,F61 | 10 | Atum | 92.70 | 29.50 | 0.54 | −20.7 | 227.4 |
5 | 2014-11-22T06h32 | F22,F23,F24,F27,F28,F51,F61 | 6.5 | Imhotep | 92.78 | 29.50 | 0.54 | −22.0 | 182.8 |
6 | 2014-09-19T09h19 | F22,F16,F23,F24,F41 | 2–5 (each) | Khepry | 70.48 | 26.50 | 0.49 | 4.2 | 71.7 |
7 | 2014-09-05T05h21 | F22,F23,F27,F16,F28,F41,F71 | 3–5 (each) | Imhotep | 57.23 | 41.44 | 0.77 | −8.1 | 188.3 |
8 | 2014-09-05T08h00 | F22,F23,F27,F16,F28,F41,F71 | 6 | Imhotep | 58.43 | 40.76 | 0.75 | −2.4 | 174.8 |
Notes. The time (UT) refers to the start time of the first image of each sequence, followed by the number of filters available. The diameter size (d) of the spots along with the location region, phase angle (α), distance between Rosetta spacecraft and comet surface (Δ), spatial resolution (R), latitude (Lat), and longitude (Long) are reported.
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