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.
| Small Delta or Fan: ESP_074848_2040 ESP_084092_2040 (Interval in Earth days: 720) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.84 | 79.8 | 6.71 | -15.1 | 64.8 | 62.0 |
| Martin Crater Central Uplift: ESP_074946_1585 ESP_075157_1585 (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 | -21.3 | 290. | -5.4 | -12.7 | 41.7 | 39.9 |
| Gullies: ESP_074803_1340 ESP_075225_1340 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.5 | 237. | 5.48 | -8.72 | 43.5 | 41.4 |
| Fossa in Orcus Patera: ESP_074739_1935 ESP_075662_1935 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.24 | 178. | -3.1 | 20.54 | 59.3 | 47.6 |
| Slope Streaks in Arabia Terra: ESP_074810_1820 ESP_075588_1820 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.851 | 41.6 | -9.5 | 3.244 | 52.5 | 42.7 |
| Conical Pit in Residual Ice Cap: ESP_074910_0925 ESP_074869_0925 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.5 | 253. | 7.56 | 25.40 | 65.2 | 63.6 |
| Mesa Stratigraphy at Terby Crater: ESP_074888_1520 ESP_083064_1520 (Interval in Earth days: 637) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 74.6 | 2.42 | -10.5 | 41.0 | 50.7 |
| Landslide Deposit in West Candor Chasma: ESP_074867_1730 ESP_067178_1730 (Interval in Earth days: 599) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.82 | 284. | 16.7 | -1.45 | 45.8 | 39.1 |
| Scarp Monitoring: ESP_074731_1225 ESP_075443_1225 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -57.0 | 47.2 | -3.5 | 8.259 | 48.8 | 45.7 |
| Channel near Huygens Crater: ESP_074915_1605 ESP_075271_1605 (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 | -19.5 | 56.8 | -2.6 | 8.28 | 42.3 | 37.6 |
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