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.
| South Polar Layered Deposits Exposed in Chasma Australe Wall: ESP_014360_0985 ESP_022694_0985 (Interval in Earth days: 649) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.3 | 95.8 | -6.3 | -20.6 | 70.7 | 65.3 |
| Ophir Chasma Interior Deposits: ESP_014352_1760 ESP_021499_1760 (Interval in Earth days: 557) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.01 | 287. | -4.3 | -21.7 | 35.5 | 51.9 |
| Araneiform Morphology: ESP_014309_0930 ESP_014440_0930 (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 | -87.0 | 72.4 | 7.05 | 20.49 | 74.1 | 75.0 |
| Trough Near Protonilus Mensae: ESP_014400_2200 ESP_022892_2200 (Interval in Earth days: 662) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.86 | 50.4 | 3.28 | -15.1 | 61.1 | 65.7 |
| Stratigraphy of Crater Pedestal: ESP_014308_1135 ESP_020690_1135 (Interval in Earth days: 497) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -66.5 | 60.3 | -7.4 | 16.19 | 58.0 | 67.9 |
| Fresh 5-Kilometer Diameter Rayed Crater: ESP_014265_1570 ESP_020845_1570 (Interval in Earth days: 512) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.6 | 144. | 4.66 | -8.29 | 33.4 | 53.3 |
| Layered Terrain between Aeolis and Zephyria Plana: ESP_014291_1770 ESP_020515_1775 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.69 | 149. | 25.6 | 3.798 | 34.0 | 54.5 |
| Large Rocky Central Uplift: ESP_014410_1470 ESP_020423_1470 (Interval in Earth days: 468) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.5 | 146. | 2.49 | -12.5 | 37.2 | 60.1 |
| 6-Kilometer Diameter Rayed Crater in Terra Sabaea: ESP_014400_1525 ESP_020703_1525 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 59.1 | 4.96 | 17.81 | 35.1 | 53.4 |
| Triple Crater Fill and Gullies: ESP_014263_1435 ESP_014329_1435 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.0 | 199. | 14.3 | -4.42 | 36.7 | 38.5 |
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