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.
| Pit in Mid-Latitude Deposit: ESP_065905_1315 ESP_066591_1315 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.3 | 109. | 1.16 | -13.6 | 46.5 | 44.1 |
| Graben and Lava Flows East of Arsia Mons: ESP_065834_1685 ESP_065768_1685 (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 | -11.1 | 242. | -8.6 | 7.596 | 49.8 | 49.3 |
| Mounds in Oxia Colles: ESP_065857_1990 ESP_065725_1990 (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 | 18.87 | 331. | -12. | 14.58 | 64.9 | 63.7 |
| Layered Bedrock: ESP_065747_1740 ESP_065958_1740 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.04 | 95.2 | 6.12 | 24.74 | 51.5 | 48.1 |
| Gullies in Crater in Nereidum Montes: ESP_066095_1350 ESP_066504_1350 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.8 | 324. | -3.4 | -24.2 | 44.1 | 43.7 |
| Central Pit Crater with Possibly Active Slope Processes: ESP_065704_1480 ESP_065770_1480 (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 | -31.6 | 191. | 7.68 | -6.72 | 46.3 | 46.6 |
| Cerberus Fossae Ripple Changes: ESP_065863_1875 ESP_065929_1875 (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 | 7.577 | 167. | 4.24 | -9.95 | 57.1 | 57.5 |
| West Rim of Impact Crater in Coprates Chasma: ESP_065832_1675 ESP_065344_1675 (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 | -12.3 | 294. | 21.2 | 11.53 | 47.2 | 52.3 |
| Well-Preserved Impact Crater: ESP_065749_1375 ESP_065195_1375 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.9 | 46.3 | -2.8 | 7.31 | 47.3 | 54.2 |
| Fans and Polygons: ESP_065786_0925 ESP_065866_0925 (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 | -87.2 | 167. | 8.69 | 2.249 | 66.3 | 66.8 |
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