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.
| North Polar Residual Cap Topography: ESP_079719_2690 ESP_079773_2690 (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 | 89.24 | 232. | -19. | -22.7 | 64.3 | 64.4 |
| Southwest Melas Chasma Slopes: ESP_079509_1680 ESP_087025_1680 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.6 | 284. | -1.8 | -14.5 | 63.4 | 55.2 |
| Traverse Ramp in East Coprates Chasma: ESP_079706_1640 ESP_079772_1640 (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 | -15.7 | 307. | 4.48 | -16.1 | 66.0 | 67.4 |
| Crater-Delineating Mounds in Chryse Planitia: ESP_079784_2055 ESP_079929_2055 (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 | 25.44 | 333. | -7.9 | 10.79 | 47.2 | 46.1 |
| Hillslope-Channel Coupling in High Drainage Density Region: ESP_079633_1610 ESP_079000_1610 (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 | -18.7 | 141. | -8.3 | 2.535 | 68.6 | 65.7 |
| Scalloped Cliff Formations : ESP_079343_2640 ESP_079237_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.86 | 111. | -8.8 | 5.451 | 59.9 | 59.4 |
| Layered Deposits: ESP_079096_2225 ESP_079241_2225 (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 | 42.08 | 32.5 | 0.36 | 11.98 | 43.4 | 42.5 |
| Terrain Sample: ESP_079080_2005 ESP_079225_2005 (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 | 20.08 | 113. | -6.5 | 9.074 | 46.5 | 45.7 |
| Segment of Valley in Tyrrhena Terra: ESP_079173_1615 ESP_080861_1615 (Interval in Earth days: 132) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.1 | 96.0 | 26.2 | 13.62 | 64.8 | 64.8 |
| Mesas in Shallow Trough in Sirenum Fossae: ESP_079340_1550 ESP_079907_1550 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.9 | 220. | -8.0 | 10.47 | 72.1 | 71.8 |
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