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.
| Dune Interaction with Residual Polar Ice: ESP_080121_2605 ESP_079673_2605 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.53 | 98.1 | 23.9 | 9.047 | 58.0 | 57.0 |
| Dune Interaction with Residual Polar Ice: ESP_080069_2605 ESP_080583_2610 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.66 | 98.6 | -8.3 | 6.294 | 59.7 | 63.1 |
| Preserved Meanders in Jezero Crater Outlet: ESP_079846_1990 ESP_079701_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 | 18.72 | 78.4 | 29.1 | 12.20 | 46.0 | 47.2 |
| Olympia Cavi Interior Scarps and Dunes: ESP_079958_2650 ESP_080076_2650 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.06 | 235. | -7.8 | 6.723 | 61.6 | 61.6 |
| Erosional Features on Olympus Mons: ESP_080078_2075 ESP_080144_2075 (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 | 27.31 | 226. | 8.64 | -7.86 | 46.4 | 48.0 |
| Defrosting Dunes in Chasma Boreale: ESP_080112_2645 ESP_080139_2645 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.55 | 336. | 8.30 | -5.70 | 61.4 | 62.2 |
| Potential Fluvial Ripples on Surface above Shalbatana Vallis: ESP_079811_1875 ESP_079877_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 | 7.589 | 318. | -2.2 | -21.2 | 53.2 | 54.8 |
| North Polar Residual Cap Topography: ESP_079851_2680 ESP_079734_2680 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.82 | 241. | -8.4 | -22.5 | 63.2 | 63.4 |
| Equatorial-Facing Trough Slope Exposure of North Polar Layered Deposits: ESP_079448_2670 ESP_079515_2670 (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 | 86.93 | 101. | -6.8 | -20.7 | 61.8 | 62.5 |
| 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 |
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