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.
| Terrain Northeast of Chryse Planitia: ESP_090214_2200 ESP_090491_2200 (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 | 39.48 | 332. | -3.6 | -16.1 | 57.8 | 62.7 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_090202_1645 ESP_090479_1645 (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 | -15.3 | 306. | 4.32 | -12.0 | 60.9 | 61.0 |
| Dune Monitoring in Nilosyrtis Mensae: ESP_090092_2110 ESP_089947_2110 (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 | 30.73 | 63.1 | 7.05 | -9.93 | 53.7 | 53.7 |
| Knobs in Arcadia Planitia: ESP_090206_2220 ESP_090483_2220 (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 | 41.62 | 189. | 5.61 | -6.01 | 57.5 | 62.4 |
| Thermal Anomaly in Lava Flows of Elysium Region: ESP_090141_1995 ESP_090497_1995 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.33 | 167. | -1.4 | 19.13 | 54.2 | 55.3 |
| Landing Site Characterization for Possible Future Rotorcraft : ESP_090127_2185 ESP_089204_2185 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.18 | 186. | 4.89 | -13.2 | 55.7 | 48.1 |
| Light-Toned Deposits in Northeast Iani Chaos: ESP_090227_1780 ESP_090794_1780 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.88 | 342. | -0.8 | -16.3 | 57.1 | 58.6 |
| Light-Toned Exposures in Capri Chasma: ESP_090215_1670 ESP_090149_1670 (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 | -12.9 | 312. | -3.4 | 16.26 | 60.6 | 59.3 |
| Inverted Channel in Noachis Terra: ESP_090252_1600 ESP_090397_1600 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.8 | 23.1 | -5.0 | 18.55 | 63.1 | 60.5 |
| Young Lava Flows in Elysium Region: ESP_090273_1975 ESP_090339_1975 (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 | 17.12 | 164. | -1.2 | -18.6 | 55.2 | 57.2 |
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