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.
| Layered Terrain on Hellas Basin Floor: PSP_007399_1385 ESP_016563_1385 (Interval in Earth days: 715) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.4 | 48.4 | -6.2 | 22.94 | 69.9 | 72.6 |
| Lineated Valley Fill in Deuteronilus Mensae: PSP_007795_2175 PSP_009588_2175 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.35 | 24.6 | -4.2 | 7.505 | 42.0 | 44.3 |
| Large Yardangs Cut by Smaller Yardangs: PSP_007460_1675 ESP_060021_1675 (Interval in Earth days: 4096) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 177. | 2.01 | -13.6 | 51.1 | 45.6 |
| Large Dunes Possibly of Aqueous Origin in Gale Crater: PSP_007356_1750 PSP_008147_1750 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.19 | 137. | -4.1 | 6.367 | 46.5 | 53.3 |
| Blocky Deposit and Valley Networks Along Melas Chasma Wallrock: PSP_007443_1705 PSP_007733_1705 (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 | -9.17 | 282. | -9.1 | 5.346 | 49.8 | 52.0 |
| Small Lava Flows Emanating From the Cerberus Fossae: PSP_007197_1910 PSP_008199_1910 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.63 | 156. | 5.84 | -4.05 | 39.2 | 46.5 |
| Unnamed Well-Preserved Crater in Terra Cimmeria: PSP_007000_1475 PSP_007145_1475 (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 | -32.0 | 141. | -1.0 | 10.11 | 57.0 | 58.6 |
| Partially-Buried Pre-Existing Crater: PSP_007524_1400 ESP_016108_1400 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 234. | -1.4 | -18.6 | 70.0 | 67.6 |
| Western Elysium Planitia Boundary: PSP_008015_1840 PSP_009940_1840 (Interval in Earth days: 150) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.067 | 141. | -0.4 | -16.9 | 47.9 | 55.3 |
| Light Outcrop in Aurorae Chaos: PSP_007705_1730 PSP_009498_1730 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.78 | 327. | -5.9 | 5.161 | 51.2 | 59.1 |
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