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.
| Light-Toned Material and Possible Unit Contact in Bakhuysen Crater Floor : ESP_046036_1575 ESP_046458_1575 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.3 | 15.5 | 6.93 | -9.07 | 58.9 | 57.3 |
| High-Latitude Exposure of North Polar Layered Deposits : ESP_045443_2690 ESP_045547_2690 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.77 | 9.66 | -26. | -21.6 | 71.3 | 72.1 |
| Eastern Ejecta of Well-Preserved 8-Kilometer Crater in Hesperia Planum : ESP_045650_1540 ESP_051821_1540 (Interval in Earth days: 481) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.7 | 115. | -1.8 | -26.9 | 63.7 | 62.2 |
| Beautiful Blocks of Bedrock: ESP_044902_1575 ESP_044968_1575 (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 | -22.1 | 13.9 | 2.01 | -16.6 | 65.0 | 65.9 |
| Scarp in Amazonis Planitia : ESP_045647_2055 ESP_046425_2055 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.47 | 191. | 0.64 | -12.9 | 45.1 | 53.8 |
| Large Alcove Dunes : ESP_045571_2565 ESP_046375_2565 (Interval in Earth days: 63) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.19 | 95.3 | -7.4 | 13.71 | 63.2 | 74.7 |
| Exposure of North Polar Layered Deposits : ESP_045474_2730 ESP_045618_2730 (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 | 87.07 | 93.0 | -8.0 | -20.6 | 72.3 | 75.4 |
| Stratified Material in Tithonium Chasma : ESP_045486_1750 ESP_062022_1750 (Interval in Earth days: 1289) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.84 | 270. | 6.77 | 24.95 | 52.1 | 54.3 |
| Impact Crater and Ejecta Partially Buried by Lobate Debris Apron : ESP_045640_2210 ESP_050901_2210 (Interval in Earth days: 410) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.60 | 21.0 | -8.8 | 6.271 | 47.8 | 44.7 |
| Exposure of North Polar Layered Deposits: ESP_045407_2660 ESP_045485_2660 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.16 | 232. | -8.8 | 5.759 | 67.9 | 68.6 |
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