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.
| Fresh-Looking Gully in Wall of Massif: PSP_003170_1330 PSP_003302_1330 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.6 | 309. | 2.89 | -27.2 | 58.7 | 58.9 |
| Gullies in Southern Latitude Crater: PSP_004145_1455 ESP_013098_1455 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.3 | 329. | -0.1 | -21.4 | 42.1 | 43.2 |
| Excellent Exposure of Basal Section of Polar Layered Deposits: PSP_003994_1080 PSP_004126_1080 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.8 | 140. | 1.67 | -13.6 | 57.1 | 56.8 |
| Crater Southwest of Herschel Crater with Dune Field: PSP_003638_1635 PSP_004350_1635 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.3 | 128. | 1.50 | 21.38 | 49.6 | 40.0 |
| Possible Small Volcano at Syria Planum: PSP_004187_1675 ESP_056787_1675 (Interval in Earth days: 4099) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 261. | -26. | -5.64 | 46.8 | 45.7 |
| Breached Impact Crater in Elysium Planitia: PSP_004151_1810 ESP_020963_1810 (Interval in Earth days: 1310) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.869 | 160. | 1.37 | -21.1 | 50.9 | 56.5 |
| Gullies in the North-Facing Wall of a Crater: PSP_003215_1405 PSP_003492_1405 (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 | -38.9 | 160. | -6.5 | -26.6 | 56.4 | 54.0 |
| Small Scallops Suggesting Sublimation O North Bank of Auqakuh Vallis: PSP_003482_2115 PSP_005895_2115 (Interval in Earth days: 188) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.05 | 60.7 | 6.34 | 26.06 | 68.8 | 48.6 |
| Layers Exposed in the Central Uplift of an Unnamed Crater: PSP_003803_1515 ESP_013679_1515 (Interval in Earth days: 770) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.3 | 304. | 5.29 | -11.0 | 46.2 | 36.5 |
| Light-Toned Outcrops in the Plains Between Melas and Candor Chasma: PSP_004318_1730 PSP_004740_1730 (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 | -6.84 | 282. | -3.1 | -15.3 | 45.8 | 41.7 |
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