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.
| 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 |
| Well-Preserved Crater in Tyrrhena Terra: ESP_025409_1615 ESP_025686_1615 (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 | -18.4 | 98.8 | 6.51 | -17.0 | 56.6 | 60.7 |
| 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 |
| 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 |
| Light-Toned Material along Coprates Chasma Wallrock: ESP_025441_1650 ESP_027973_1650 (Interval in Earth days: 198) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 304. | 9.23 | -16.1 | 54.3 | 61.4 |
| Terra Sabaea Intracrater Bedform Changes Changes: ESP_025794_1750 ESP_026427_1750 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.07 | 26.0 | 18.4 | -1.81 | 50.8 | 55.5 |
| 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 |
| 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 |
| Bedrock Exposed in the Central Uplift of a Unnamed Crater: ESP_025766_2005 ESP_025700_2005 (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 | 20.18 | 69.3 | -7.5 | 11.70 | 41.5 | 39.7 |
| Source of Flow Visible in CTX Image P20_008700_1787: ESP_025697_1805 ESP_037169_1805 (Interval in Earth days: 894) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.572 | 155. | -6.8 | 8.034 | 48.6 | 54.9 |
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