Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Sedimentary Fans in Crater : ESP_050790_1400 ESP_058821_1400 (Interval in Earth days: 625) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.8 | 182. | 7.54 | -2.73 | 55.4 | 43.1 |
| Candidate Red Dragon Landing Site : ESP_050868_2200 ESP_050934_2200 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.82 | 202. | 5.82 | -10.8 | 44.5 | 45.1 |
| Well-Preserved 7-Kilometer Impact Crater : ESP_050726_1595 ESP_059403_1595 (Interval in Earth days: 676) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.2 | 128. | -8.4 | 14.49 | 42.5 | 39.0 |
| Well-Preserved Crater : ESP_050586_1335 ESP_050863_1335 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.3 | 353. | 2.21 | -22.7 | 57.1 | 63.2 |
| The Niagara Falls of Mars: ESP_050406_1585 ESP_050472_1585 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.3 | 223. | 19.5 | -4.75 | 36.7 | 39.2 |
| Monitoring Sand Sheets and Dunes: ESP_050182_1165 ESP_050261_1165 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -63.3 | 228. | -0.4 | 16.79 | 63.8 | 64.3 |
| Knob and Flows in Adamas Labyrinthus : ESP_050252_2165 ESP_050542_2165 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.05 | 102. | -6.6 | 10.74 | 49.2 | 44.9 |
| Deposit on Crater Floor : ESP_050147_1560 ESP_050358_1560 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.6 | 96.3 | 6.21 | -8.55 | 35.4 | 39.1 |
| Gully Monitoring : ESP_050263_1420 ESP_050553_1420 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.8 | 171. | 1.08 | 20.24 | 45.6 | 49.3 |
| Search for Active Glacial Flow: ESP_050279_1420 ESP_050490_1420 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.8 | 95.4 | -8.5 | -19.1 | 46.5 | 50.6 |
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