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.
| Lava Flows in Crater in Southwestern Daedalia Planum : ESP_028886_1560 ESP_029031_1560 (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 | -23.9 | 220. | -6.7 | 8.729 | 59.9 | 57.6 |
| Depositional Fan on Northern Rim of Hargraves Crater : ESP_028746_2010 ESP_033427_2010 (Interval in Earth days: 365) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.00 | 75.5 | 8.50 | -7.28 | 53.5 | 38.7 |
| Small Fresh Crater : ESP_028795_2305 ESP_037155_2305 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.08 | 174. | -1.2 | -20.5 | 63.8 | 59.6 |
| Troughs and Small Cones in Cydonia Region : ESP_028670_2225 ESP_037465_2225 (Interval in Earth days: 685) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.35 | 349. | -6.3 | 4.464 | 59.2 | 59.5 |
| Chevrons on Lava Surface in Marte Vallis : ESP_028716_1880 ESP_053704_1875 (Interval in Earth days: 1947) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.810 | 177. | 0 | 12.89 | 53.4 | 47.2 |
| Layering in Crater in Mawrth Vallis : ESP_028855_2045 ESP_020297_2045 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.23 | 341. | -13. | -25.2 | 57.0 | 61.1 |
| Light-Toned Deposits in Ladon Valles Basin : ESP_028816_1605 ESP_029594_1605 (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 | -19.2 | 329. | 6.81 | -3.96 | 57.8 | 53.2 |
| Well-Preserved Double Crater : ESP_028631_1965 ESP_028776_1965 (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 | 16.16 | 336. | -1.4 | 11.21 | 53.0 | 53.0 |
| Lava Flow Through Breached Crater Rim in Tartarus Montes : ESP_028637_2040 ESP_029072_2040 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.67 | 172. | -8.4 | 27.76 | 54.3 | 55.5 |
| Crater Filled with Mantling Deposit in Far Eastern Acidalia Planitia : ESP_028628_2315 ESP_028694_2315 (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 | 51.20 | 54.1 | -4.9 | -17.8 | 61.8 | 64.0 |
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