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.
| Small Crater with Layered Fill in Schiaparelli Crater: PSP_007400_1790 PSP_007756_1790 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.75 | 14.3 | 9.35 | -3.82 | 44.1 | 48.4 |
| Possible Chloride Salt Deposit: PSP_007058_1745 ESP_016354_1745 (Interval in Earth days: 724) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.62 | 353. | 4.05 | -22.5 | 42.7 | 49.8 |
| Recent 6-Kilometer Diameter Crater in Acidalia Planitia: PSP_007982_2125 ESP_015933_2125 (Interval in Earth days: 620) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.28 | 318. | -3.1 | 18.34 | 41.4 | 40.0 |
| Light-Toned Layering in Melas Chasma: PSP_007812_1700 PSP_010660_1700 (Interval in Earth days: 222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.87 | 285. | 5.77 | -12.6 | 53.1 | 60.5 |
| Diverse Features in Utopia Region: PSP_007951_2220 PSP_008162_2220 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.58 | 82.8 | 6.93 | -5.86 | 41.7 | 42.5 |
| Impact Crater on the Floor of Kasei Valles: PSP_007218_2055 ESP_052750_2055 (Interval in Earth days: 3548) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.32 | 300. | 8.56 | 20.78 | 39.1 | 38.2 |
| Reull Vallis: PSP_007819_1390 PSP_009612_1390 (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 | -40.6 | 99.6 | -6.4 | 7.67 | 74.7 | 81.0 |
| Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin: PSP_007377_1700 PSP_008379_1700 (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 | -9.82 | 283. | 5.56 | -6.99 | 48.4 | 58.5 |
| Fresh 7-Kilometer Diameter Crater with Bright Rayed Ejecta: PSP_007731_2060 ESP_026310_2060 (Interval in Earth days: 1448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.77 | 333. | 1.95 | 28.52 | 40.6 | 38.7 |
| Crater with Gullies: PSP_007652_2230 ESP_024095_2230 (Interval in Earth days: 1282) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.65 | 328. | -6.0 | -27.7 | 43.8 | 52.7 |
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