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 Region of Past Ponded Water: ESP_014407_2045 ESP_020288_2045 (Interval in Earth days: 458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.15 | 221. | 5.35 | 29.18 | 49.2 | 56.3 |
| 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 |
| 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 |
| Tractus Catena: ESP_014432_2110 ESP_023135_2110 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.77 | 257. | 5.46 | -19.5 | 53.6 | 55.4 |
| 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 |
| 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 |
| 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 |
| Exposures of Layered Rocks in Argyre Region: ESP_014167_1300 ESP_021947_1300 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.7 | 302. | 8.10 | -18.2 | 43.7 | 44.1 |
| Ferric Oxide-Rich Deposit in East Candor Chasma: ESP_014154_1730 ESP_014431_1730 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.75 | 292. | 5.69 | -21.1 | 35.2 | 35.9 |
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