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.
| Surface Features of Debris Apron in Deuteronilus Mensae : ESP_046787_2210 ESP_090199_2210 (Interval in Earth days: 3382) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.80 | 23.8 | 7.56 | -18.2 | 62.6 | 59.2 |
| Small Dome and Barchan Dunes in Newton Crater : ESP_046649_1385 ESP_046504_1385 (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 | -41.1 | 202. | 2.56 | -11.2 | 62.5 | 65.3 |
| Candidate Recent Impact Site : ESP_046707_2220 ESP_055146_2220 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.45 | 48.7 | -1.4 | -21.1 | 62.4 | 59.2 |
| Youthful Dark Rayed Crater with Boulders in Primary Ejecta Deposit : ESP_046618_1770 ESP_047330_1770 (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 | -3.07 | 324. | -8.1 | 2.309 | 52.2 | 51.0 |
| Northern Ejecta and Rays of Istok Crater : ESP_046686_1350 ESP_064580_1350 (Interval in Earth days: 1394) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.8 | 274. | -5.2 | 19.11 | 64.4 | 62.9 |
| Monitor Seasonal Changes at South Polar Cracked and Gullied Site : ESP_046892_0980 ESP_046945_0980 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.6 | 66.2 | 4.68 | -8.76 | 81.2 | 81.2 |
| Lava Crust and Wakes in Amazonis Planitia : ESP_046675_2090 ESP_064002_2090 (Interval in Earth days: 1350) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.74 | 204. | -7.0 | 15.14 | 57.2 | 56.2 |
| Possible Phyllosilicates in Knob-Type Feature North of Hellas Planitia : ESP_046601_1580 ESP_064706_1580 (Interval in Earth days: 1411) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.9 | 71.1 | -5.0 | 21.42 | 55.8 | 55.7 |
| Cratered Layered Terrain and Wall Slopes in Melas Chasma : ESP_046725_1685 ESP_046448_1685 (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 | -11.2 | 285. | -11. | 16.82 | 53.1 | 51.8 |
| Ice-Rich Deposits in Ancient Valleys : ESP_046716_1415 ESP_064742_1415 (Interval in Earth days: 1405) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.2 | 172. | 6.21 | -3.51 | 60.1 | 60.2 |
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