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.
| Crater: ESP_016225_2355 ESP_016502_2355 (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 | 55.29 | 264. | 1.34 | -12.8 | 50.1 | 49.1 |
| Distinct Spur and Gully Mesa in Candor Chasma: ESP_016185_1740 ESP_016330_1740 (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 | -6.09 | 285. | 8.13 | 23.94 | 46.0 | 46.4 |
| Pits North of Alba Patera: ESP_016080_2310 ESP_016581_2310 (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 | 50.58 | 264. | 0 | 15.86 | 48.7 | 44.2 |
| Coprates Chasma: ESP_016211_1655 ESP_016844_1655 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 296. | 0 | -14.2 | 51.1 | 58.7 |
| Potential MSL Landing Site in Eberswalde Crater: ESP_016065_1560 ESP_016210_1560 (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 | -23.9 | 326. | -28. | -15.6 | 57.2 | 58.1 |
| Possible Bedrock Fault Northwest of Hellas Region: ESP_016180_1515 ESP_016325_1515 (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 | -28.1 | 64.6 | 6.69 | 21.45 | 59.2 | 60.2 |
| Small Volcano in THEMIS Image V19499026: ESP_016199_1940 ESP_016476_1940 (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 | 13.78 | 260. | 4.43 | -22.1 | 39.8 | 43.5 |
| Young Fluvial Valleys on Floor of Lyot Crater: ESP_016260_2295 ESP_016339_2295 (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 | 49.00 | 30.7 | 0.12 | 21.90 | 46.7 | 44.4 |
| Cliffs in Coprates Chasma: ESP_016198_1695 ESP_016343_1695 (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 | -10.4 | 291. | -1.4 | 15.71 | 49.0 | 49.5 |
| Lineated Valley Fill Near Deuteronilus Region: ESP_016168_2180 ESP_024594_2180 (Interval in Earth days: 656) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.78 | 23.8 | 4.56 | -7.15 | 42.2 | 43.8 |
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