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.
| 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 |
| 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 |
| Exposure of Polar Layered Deposits with Knobs in Places: ESP_014292_1070 ESP_014345_1070 (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 | -73.0 | 139. | -4.9 | -28.3 | 62.6 | 65.0 |
| Spiders in a Variety of Terrains: ESP_014282_0930 ESP_014413_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 | 86.5 | 8.64 | 22.23 | 73.6 | 74.5 |
| Possible Kieserite-Rich Terrain in Hebes Chasma: ESP_014418_1790 ESP_019864_1790 (Interval in Earth days: 425) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.18 | 284. | 1.76 | -16.7 | 35.6 | 56.2 |
| Western Ejecta of Zumba Crater: ESP_014262_1510 ESP_020486_1510 (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 | -28.6 | 226. | 3.35 | -17.8 | 34.8 | 58.8 |
| Pedestal Crater Stratigraphy: ESP_014295_1085 ESP_021956_1085 (Interval in Earth days: 597) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.3 | 54.2 | 7.11 | 28.62 | 60.8 | 52.1 |
| Curving End of Chasma Australe Wall: ESP_014373_0995 ESP_022918_0995 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.3 | 92.8 | 5.88 | -13.6 | 69.2 | 66.4 |
| 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 |
| 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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