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.
| Apollinaris Sulci Ancient Dunes: ESP_060166_1675 ESP_060443_1675 (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 | -12.5 | 177. | 6.46 | -16.4 | 46.1 | 51.1 |
| Small Crater in Light Mantle: ESP_060135_2350 ESP_059647_2350 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.53 | 298. | -20. | -5.52 | 51.5 | 55.6 |
| Exit Breach in Small Crater: ESP_059976_1600 ESP_060121_1600 (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 | -19.5 | 326. | -4.1 | 14.60 | 48.4 | 49.3 |
| Candidate Landing Site for 2020 Mission Near Jezero Crater: ESP_060196_1985 ESP_060486_1985 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.26 | 77.1 | -17. | 18.20 | 38.5 | 36.7 |
| Rhythmic Layers East of Medusae Fossae: ESP_057092_1770 ESP_057303_1770 (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 | -2.89 | 215. | -6.6 | 7.217 | 46.5 | 43.4 |
| Terrain in Utopia Planitia : ESP_059760_2120 ESP_060182_2120 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.46 | 96.8 | -2.6 | -7.88 | 40.3 | 39.4 |
| Well-Preserved Impact Crater : ESP_059565_1375 ESP_076393_1375 (Interval in Earth days: 1311) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.1 | 30.0 | -2.2 | 8.829 | 57.1 | 46.1 |
| Valleys in Crater Northeast of Argyre Planitia : ESP_059501_1500 ESP_060134_1500 (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 | -29.6 | 335. | 1.19 | -10.1 | 47.0 | 57.7 |
| Scarps in Icaria Region : ESP_059716_1425 ESP_059993_1425 (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 | -37.1 | 227. | -3.5 | -24.4 | 56.1 | 61.8 |
| Mass Wasting Feature on Southern Wall of Crater Near Amazonis Mensa : ESP_059611_1860 ESP_060244_1860 (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 | 5.755 | 207. | 5.84 | -4.61 | 33.9 | 39.7 |
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