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.
| Junction of Three Polar Troughs: PSP_010030_2670 PSP_010532_2670 (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 | 86.74 | 162. | -8.8 | -21.4 | 67.2 | 74.3 |
| Exposure of North Polar Basal Unit: PSP_009945_2645 PSP_010063_2645 (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 | 84.40 | 343. | -12. | 3.559 | 65.2 | 65.5 |
| Western Rim and Ejecta of Very Young 12-Kilometer Diameter Crater: PSP_009810_2140 PSP_010443_2140 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.45 | 84.2 | 7.72 | -5.93 | 45.6 | 51.8 |
| Pit and Channel on Southwestern Pavonis Mons: PSP_009923_1785 PSP_010213_1785 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.67 | 246. | -21. | 14.06 | 58.1 | 55.7 |
| Distributaries From Athabasca Valles: PSP_009768_1880 PSP_010045_1880 (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 | 7.721 | 154. | 7.98 | -19.7 | 51.6 | 54.3 |
| Potential Paleolake in Crater in Ophir Planum: PSP_010290_1700 PSP_010435_1700 (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 | -10.0 | 306. | 0.86 | 17.82 | 60.3 | 58.8 |
| Well-Preserved Crater on a Steep Slope in Tyrrhena Terra: PSP_009824_1610 PSP_010246_1610 (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 | -18.5 | 69.0 | 6.12 | -5.57 | 65.8 | 65.3 |
| Tooting Crater Southern Ejecta Layer: PSP_009766_2030 PSP_009832_2030 (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 | 22.53 | 207. | 2.91 | -16.9 | 47.2 | 49.2 |
| Volcanic Fissure Vent in Elysium Planitia: PSP_010269_1900 PSP_010414_1900 (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 | 9.630 | 157. | -2.2 | 14.68 | 52.9 | 52.0 |
| Stratigraphy of the North Polar Deposits: PSP_010198_2645 PSP_010014_2645 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.38 | 253. | 7.14 | -7.89 | 66.8 | 65.5 |
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