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.
| Very Fresh Unnamed Crater in Tyrrhena Terra: PSP_010852_1735 ESP_051743_1735 (Interval in Earth days: 3186) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.41 | 81.6 | 6.01 | -16.4 | 57.8 | 48.3 |
| Very Fresh Small Crater at 48 North Latitude: PSP_010638_2280 ESP_051951_2280 (Interval in Earth days: 3219) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.60 | 157. | 2.16 | -18.8 | 56.3 | 43.7 |
| Light-Toned Bedrock Exposed in Walls and Central Peak of Crater: ESP_011314_1585 ESP_011591_1585 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 70.0 | 5.84 | -21.8 | 60.4 | 60.7 |
| Stratigraphy of Primary Mesa in Terby Crater: PSP_010826_1525 ESP_016272_1525 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 74.2 | 4.13 | -10.0 | 65.9 | 60.7 |
| Crater with Extensive Ejecta Deposits: PSP_010611_2210 ESP_027173_2210 (Interval in Earth days: 1290) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.51 | 175. | 0.50 | -12.9 | 54.2 | 44.1 |
| Diverse Hydrated Silicates Near Atlantis Chaos: PSP_010822_1445 ESP_063291_1445 (Interval in Earth days: 4089) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.2 | 184. | 2.16 | 23.10 | 70.0 | 71.3 |
| Complex Morphology in Acidalia Region: ESP_011384_2185 ESP_011661_2185 (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 | 38.01 | 310. | 7.35 | -13.2 | 63.5 | 68.9 |
| Possible Chloride Salt Deposits Observed in THEMIS: PSP_010597_1470 PSP_007380_1470 (Interval in Earth days: 251) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.7 | 205. | 18.1 | -6.34 | 69.5 | 63.4 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010808_2720 ESP_028150_2680 (Interval in Earth days: 1351) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.93 | 95.5 | -6.3 | -11.4 | 79.4 | 74.3 |
| Central Uplift of a Large Impact Crater: PSP_010534_1620 ESP_051992_1620 (Interval in Earth days: 3230) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.8 | 125. | -4.5 | -24.2 | 63.7 | 58.4 |
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