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.
| Fan-Shaped Deposit in Arcadia Planitia: ESP_089428_2200 ESP_089494_2200 (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 | 39.86 | 188. | 6.33 | -9.62 | 48.3 | 50.2 |
| Large Crater on Slope of Layered Deposits: ESP_089517_1735 ESP_089095_1735 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.23 | 287. | -20. | -5.59 | 60.6 | 59.8 |
| Features around Crater in Arabia Terra: ESP_089592_2190 ESP_089104_2190 (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 | 38.44 | 34.3 | -16. | 10.19 | 51.6 | 45.4 |
| Light-Toned Deposits in Iani Chaos: ESP_089383_1780 ESP_089871_1780 (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 | -1.75 | 341. | 18.5 | -11.7 | 55.6 | 57.9 |
| Potential Compound Dune: ESP_089573_2610 ESP_089389_2610 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.87 | 160. | 19.2 | -5.86 | 64.3 | 63.7 |
| Curve in Valley in Northern Terra Cimmeria: ESP_089390_1675 ESP_089535_1675 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.4 | 154. | -8.8 | 8.148 | 63.0 | 61.6 |
| Planned ExoMars Landing Ellipse Imaging in Oxia Planum: ESP_089581_1995 ESP_089291_1995 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.24 | 335. | 3.28 | -24.9 | 50.3 | 51.5 |
| Sample of Scalloped Terrain West of Erebus Montes: ESP_089349_2195 ESP_089072_2195 (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 | 39.37 | 187. | -8.3 | 14.20 | 48.9 | 44.9 |
| Thermal Anomaly in Young Lava Flows of Elysium Region: ESP_089284_1970 ESP_089429_1970 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.03 | 163. | 2.69 | 16.88 | 49.6 | 48.9 |
| Potential Compound Dune: ESP_089362_2590 ESP_089415_2590 (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 | 78.72 | 174. | 6.27 | -7.76 | 61.5 | 63.0 |
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