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.
| Possible MSL Rover Landing Site: Edge of Fan in Bakhuysen Crater: PSP_005686_1575 ESP_011382_1575 (Interval in Earth days: 444) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.3 | 16.2 | 0.57 | -23.2 | 34.1 | 62.4 |
| Proposed MSL Site in Terby Crater: PSP_005618_1525 PSP_006752_1525 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 73.5 | -0.9 | -18.2 | 35.2 | 51.3 |
| Slope Streaks within an Impact Crater in Terra Sabaea: PSP_005369_1925 PSP_005514_1925 (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 | 12.20 | 26.3 | 3.14 | 16.92 | 43.7 | 41.2 |
| Negative and Positive Relief Valley Features: PSP_005355_2125 ESP_084304_2125 (Interval in Earth days: 6152) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.14 | 45.9 | 1.83 | 17.86 | 58.1 | 63.9 |
| Impact Crater Cut by Ganges Chasma: PSP_005543_1725 ESP_011595_1725 (Interval in Earth days: 471) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.60 | 318. | -2.2 | -18.1 | 33.8 | 58.9 |
| Uzboi Vallis Breach in Holden Crater Rim: PSP_003288_1530 PSP_003710_1530 (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 | -26.9 | 325. | 0 | -11.1 | 52.9 | 48.7 |
| Interior of Western Candor Chasma: PSP_003474_1735 PSP_003540_1735 (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 | -6.44 | 283. | 17.0 | -6.73 | 51.8 | 53.2 |
| Layered Deposits in Terby Crater: PSP_001662_1520 PSP_002572_1520 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 74.2 | -3.0 | -17.3 | 67.8 | 61.8 |
| Light-toned Layering on Plains South of the West Candor Region: PSP_005096_1730 PSP_005241_1730 (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 | -6.93 | 283. | -12. | 2.319 | 37.7 | 35.4 |
| Faulting within the Layered Deposits in Candor Chasma: PSP_001641_1735 PSP_002063_1735 (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 | -6.67 | 284. | -1.8 | 23.61 | 57.4 | 54.8 |
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