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.
| Branching Ridges: ESP_025683_1900 ESP_025538_1900 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.786 | 174. | 14.4 | -4.30 | 42.7 | 43.3 |
| Interactions between Crater Ejecta Mantling Deposits and Flows: ESP_025486_1805 ESP_034756_1805 (Interval in Earth days: 722) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.550 | 155. | -6.8 | -21.0 | 47.0 | 52.5 |
| Well Preserved 7-Kilometer Impact Crater in Utopia Planitia: ESP_025791_1945 ESP_025646_1945 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.46 | 104. | 24.6 | 6.969 | 40.6 | 41.4 |
| Ridges or Flows in Northeast Gale Crater: ESP_025790_1750 ESP_027135_1750 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.71 | 137. | -6.0 | 3.949 | 52.2 | 55.9 |
| Olympus Mons Bedform Change Detections: ESP_025536_1990 ESP_024824_1990 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.84 | 227. | -3.2 | -23.8 | 40.5 | 39.4 |
| Abalos Mensa and Abalos Scopuli Region: ESP_025665_2610 ESP_025718_2610 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.01 | 280. | 7.35 | -3.58 | 60.5 | 60.6 |
| Flow Draped over Crater Rim Visible in CTX Image : ESP_025563_1975 ESP_025207_1975 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.48 | 209. | 15.2 | 2.131 | 39.4 | 38.8 |
| Reticulate Bedform Change Detection Northwest Ascraeus Mons: ESP_025667_1960 ESP_026168_1960 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.83 | 252. | -8.4 | 18.74 | 42.3 | 42.3 |
| Contact between Yardang-Forming Material and Platy Flow Material: ESP_025473_1840 ESP_034255_1840 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.897 | 149. | -3.9 | 28.53 | 45.2 | 43.3 |
| Channel in Tharsis Region: ESP_025417_1965 ESP_024916_1965 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.19 | 235. | 17.6 | -8.13 | 38.8 | 38.5 |
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