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.
| Tooting Crater Southern Ejecta Layer: PSP_009766_2030 PSP_009832_2030 (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 | 22.53 | 207. | 2.91 | -16.9 | 47.2 | 49.2 |
| Basal Unit and North Polar Layered Deposits in Chasma Boreale Scarp: PSP_009995_2650 PSP_010128_2650 (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 | 85.06 | 0.70 | 19.4 | 5.177 | 65.3 | 66.6 |
| Central Uplift of Hargraves Crater in the Nili Fossae Region: PSP_009639_2010 PSP_010272_2010 (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 | 20.73 | 75.8 | -5.4 | -21.0 | 47.8 | 52.1 |
| Flow Lobes in Northern Plains Crater: PSP_009803_2505 PSP_009935_2505 (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 | 70.28 | 266. | 4.45 | -8.78 | 54.9 | 57.1 |
| Possible Pingos in Gusev Crater: PSP_009385_1655 PSP_009886_1655 (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 | -14.2 | 175. | -18. | 5.226 | 65.1 | 63.0 |
| Hydrated Light-Toned Layers on Crater Floor: PSP_010274_2140 PSP_010696_2140 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.63 | 17.0 | 5.05 | -8.32 | 49.3 | 54.8 |
| Exposure of North Polar Layered Deposits for Stratigraphic Analysis: PSP_009471_2670 PSP_009683_2670 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.93 | 301. | -8.2 | -21.8 | 63.0 | 65.1 |
| Exposure of Polar Layered Deposits on Ridges and Troughs: PSP_009969_2630 PSP_010008_2630 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.92 | 40.8 | -1.7 | 15.24 | 63.7 | 63.3 |
| Slope Streaks on Nicholson Crater Mound: PSP_009371_1800 PSP_009516_1800 (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 | -0.00 | 195. | -5.9 | 9.471 | 55.9 | 55.0 |
| Central Peak and Pit with Bedrock Exposures: PSP_010389_1670 ESP_025751_1670 (Interval in Earth days: 1197) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.9 | 123. | 4.69 | -15.0 | 61.2 | 57.5 |
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