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.
| Abalos Mensa and Abalos Scopuli Region: ESP_025665_2610 ESP_025718_2610 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.01 | 280. | 7.35 | -3.58 | 60.5 | 60.6 |
| Wrinkle Ridge Superimposed on Well-Preserved Crater: ESP_025468_1640 ESP_024835_1640 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.7 | 288. | -5.8 | 12.96 | 56.2 | 47.5 |
| Reticulate Bedform Change Detection Northwest Ascraeus Mons: ESP_025667_1960 ESP_026168_1960 (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 | 15.83 | 252. | -8.4 | 18.74 | 42.3 | 42.3 |
| Light-Toned Material and Dark Dunes and Gullies: ESP_025177_2145 ESP_026245_2145 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.12 | 306. | 2.29 | 29.34 | 39.6 | 37.3 |
| Floor of Toro Crater: ESP_025344_1970 ESP_025067_1970 (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 | 17.00 | 71.7 | -24. | 0.616 | 41.9 | 38.4 |
| Daedalia Planum Reticulate Bedform Changes: ESP_025233_1610 ESP_025088_1610 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.6 | 223. | 13.9 | -2.92 | 54.3 | 53.5 |
| Mawrth Region Crater with Possible Sedimentary Features: ESP_025123_2045 ESP_026811_2045 (Interval in Earth days: 131) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.24 | 340. | 12.4 | -19.9 | 37.4 | 44.7 |
| Possible Phyllosilicates Northwest of Hellas Region: ESP_025107_1535 ESP_034232_1535 (Interval in Earth days: 711) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.2 | 64.5 | 7.13 | -6.50 | 58.2 | 63.5 |
| Slope Streaks in Pettit Crater: ESP_025287_1920 ESP_025643_1925 (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 | 12.20 | 186. | 0 | 14.88 | 40.5 | 41.5 |
| Fresh Crater on Northern Plains: ESP_025366_2305 ESP_025498_2305 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.19 | 184. | -3.4 | -26.3 | 45.0 | 46.4 |
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