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.
| Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor: ESP_027771_1640 ESP_028470_1640 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.7 | 56.6 | 8.78 | -7.44 | 61.0 | 59.4 |
| Flow Lobes Resting on the Elevated Platform of a Moated Crater: ESP_027708_1815 ESP_027985_1815 (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 | 1.526 | 334. | 6.95 | -8.68 | 52.4 | 53.7 |
| Tilted Block on Olympus Mons Scarp: ESP_027712_2035 ESP_028279_2035 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.21 | 223. | -6.3 | 15.88 | 47.0 | 49.0 |
| Possible Future Landing Site in Sabrina Vallis Outlet: ESP_027656_1920 ESP_027168_1920 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.87 | 313. | -3.6 | 13.23 | 49.2 | 46.9 |
| Layered Floor of Noctis Labyrinthus: ESP_027592_1685 ESP_027526_1685 (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 | -11.2 | 263. | -8.8 | 12.08 | 60.0 | 58.8 |
| Secondary Crater Chain in Cerberus Region: ESP_027741_1850 ESP_043433_1850 (Interval in Earth days: 1222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.837 | 153. | 0 | -13.8 | 51.5 | 47.5 |
| North Polar Gypsum Dunes: ESP_027595_2625 ESP_027555_2625 (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 | 82.60 | 157. | -6.6 | 8.224 | 63.7 | 62.5 |
| North Polar Gypsum Dune Changes: ESP_027713_2615 ESP_027739_2615 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.63 | 178. | -6.6 | 7.683 | 64.3 | 63.8 |
| Small Crater on North Polar Layered Deposits: ESP_027780_2680 ESP_027452_2680 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.75 | 120. | -11. | -27.3 | 69.4 | 67.0 |
| Fluvial Erosion and Resistant Layering along Canyon Wall: ESP_027552_1735 ESP_027275_1735 (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 | -6.54 | 274. | -0.8 | 18.50 | 57.0 | 55.9 |
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