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.
| Baldet Crater Dune Changes: ESP_080229_2030 ESP_080295_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 | 22.68 | 65.8 | 1.70 | -15.0 | 48.5 | 50.2 |
| Aram Chaos: ESP_080285_1830 ESP_080351_1830 (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 | 2.757 | 338. | 16.3 | -2.05 | 54.8 | 56.3 |
| Ice-Rich Deposits in Arabia Terra: ESP_080204_2145 ESP_080138_2145 (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 | 34.14 | 27.7 | -8.5 | 6.219 | 47.6 | 46.0 |
| Athabasca Valles: ESP_080450_1890 ESP_080951_1890 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.124 | 155. | -7.0 | 8.08 | 54.1 | 54.1 |
| Dune Interaction with Residual Polar Ice: ESP_080372_2605 ESP_080280_2605 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.58 | 98.0 | 7.78 | -6.43 | 60.8 | 61.0 |
| Light-Toned Exposures near Voeykov Crater: ESP_080340_1465 ESP_080274_1465 (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 | -33.0 | 283. | -1.3 | 15.81 | 77.0 | 76.2 |
| Possible Dipping Layers in Ice-Affected Crater: ESP_080515_2115 ESP_080805_2115 (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 | 31.38 | 178. | -3.2 | 15.42 | 49.2 | 49.7 |
| Floor of East Coprates Chasma: ESP_080471_1650 ESP_080972_1650 (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 | -15.0 | 304. | 7.33 | 20.06 | 64.8 | 62.3 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_080576_2395 ESP_080286_2395 (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 | 59.33 | 302. | 24.5 | 7.497 | 51.7 | 50.5 |
| Terrain Sample in Cydonia Region: ESP_080535_2210 ESP_080970_2210 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.76 | 350. | 0 | 24.49 | 49.3 | 51.2 |
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