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.
| 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 |
| A Youthful Crater in the Cydonia Colles Region: ESP_025716_2200 ESP_027417_2200 (Interval in Earth days: 132) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.64 | 350. | 4.65 | 24.57 | 39.9 | 42.0 |
| 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 |
| An Impact Crater on Upper Rim Valles Marineris: ESP_025705_1675 ESP_025560_1675 (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 | -12.3 | 298. | -0.6 | -20.3 | 55.9 | 55.8 |
| 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 |
| 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 |
| Ring-Shaped Feature in Northeastern Acidalia Region: ESP_025663_2280 ESP_026362_2280 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.84 | 355. | 4.36 | -18.8 | 42.2 | 43.4 |
| Western Portion of Well-Preserved Impact Crater: ESP_025507_1825 ESP_025863_1825 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.450 | 301. | 3.84 | 21.96 | 45.5 | 46.7 |
| Small Crater on Pedestal Crater: ESP_025776_2320 ESP_026422_2320 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.57 | 151. | -1.2 | 21.35 | 43.6 | 40.8 |
| 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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