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.
| Sapping Features East of Tooting Crater: PSP_010333_2025 PSP_010689_2025 (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 | 22.14 | 208. | -3.9 | 0.754 | 50.8 | 53.1 |
| Stratigraphy Exposed in Ausonia Cavus: PSP_009889_1480 ESP_079872_1480 (Interval in Earth days: 5452) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.7 | 96.8 | -1.5 | 12.44 | 74.4 | 76.4 |
| Small Shield Covering the Noctis Fossae: PSP_010305_1780 PSP_010661_1780 (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 | -1.91 | 256. | -7.0 | -0.74 | 57.3 | 56.9 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010153_2675 PSP_010603_2675 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.58 | 25.7 | -8.4 | -23.4 | 69.2 | 76.0 |
| Gullies in North Mid-Latitude Crater: PSP_009744_2305 PSP_010245_2305 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.11 | 84.3 | -0.6 | 14.78 | 47.4 | 50.9 |
| Fresh 8-Kilometer Diameter Impact Crater: PSP_009625_1900 ESP_016060_1900 (Interval in Earth days: 501) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.793 | 98.5 | 4.97 | -22.4 | 50.7 | 41.9 |
| Double Crater on Cerberus Plains: PSP_009860_1805 ESP_042892_1805 (Interval in Earth days: 2574) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.433 | 164. | -5.2 | -19.3 | 56.0 | 46.7 |
| Light-Toned Deposits and Possible Fluvial Channels on Floor of Ius Chasma: PSP_010146_1720 PSP_010568_1720 (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 | -7.96 | 277. | -4.7 | -18.8 | 59.9 | 60.5 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010163_2675 PSP_010230_2675 (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 | 87.26 | 123. | -8.3 | -20.4 | 69.1 | 70.5 |
| Mamers Valles: PSP_009773_2165 ESP_053789_2165 (Interval in Earth days: 3429) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.13 | 14.3 | 5.21 | -4.42 | 45.5 | 42.7 |
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