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.
| Light-Toned Layered Material in South Galle Crater : PSP_002866_1280 ESP_064565_1280 (Interval in Earth days: 4808) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -51.8 | 329. | 1.76 | -20.3 | 65.6 | 68.7 |
| Very Interesting Circular Layered Form -Crater Filled with Layered Deposits: PSP_001981_1825 PSP_002258_1825 (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 | 2.263 | 3.53 | 4.45 | -24.2 | 54.1 | 57.0 |
| Iani Chaos Light-Toned Sedimentary Layers: PSP_002206_1760 PSP_002628_1760 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.17 | 341. | 4.82 | -8.82 | 55.6 | 56.4 |
| Dark-Toned Unit Exposed atop Crater Ejecta in Meridiani Planum : PSP_002680_1825 PSP_003392_1825 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.240 | -0.3 | 7.78 | 29.45 | 55.2 | 53.5 |
| Rayed Crater: PSP_001660_1950 PSP_002570_1950 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.87 | 123. | -1.8 | -15.8 | 51.1 | 57.9 |
| Gullies on South Rim of Crater in Terra Sirenum Area: PSP_002568_1335 PSP_003201_1335 (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 | -46.4 | 184. | -1.5 | -15.7 | 67.9 | 59.4 |
| Strange Dendritic Relief Features: PSP_001950_2090 PSP_002240_2090 (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 | 28.69 | 126. | -1.5 | 23.36 | 53.0 | 53.9 |
| Tributary of Shalbatana Vallis, As Seen in MOC Image R09-01983: PSP_001930_1835 PSP_002431_1835 (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 | 3.411 | 316. | -0.0 | 24.34 | 54.1 | 53.1 |
| Contact Between Layering in Plains and Wallrock Near Ius Chasma : PSP_002459_1715 PSP_003092_1715 (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 | -8.30 | 275. | -0.0 | -21.4 | 56.4 | 56.3 |
| Gullies on Very High Dune Slip Face in Russell Crater: PSP_001440_1255 PSP_001981_1255 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.2 | 12.9 | 8.51 | -8.06 | 85.4 | 80.5 |
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