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.
| Abrading Dome Dunes in the North Polar Erg: PSP_009295_2565 PSP_009743_2565 (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 | 76.17 | 95.3 | -6.2 | 15.45 | 55.6 | 56.7 |
| Polygons and Sublimation Structures in West Utopia Planitia: PSP_008913_2255 PSP_008979_2255 (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 | 45.20 | 92.5 | 5.21 | -12.6 | 42.4 | 44.1 |
| Well-Preserved 9-Kilometer Diameter Crater: PSP_008902_1565 PSP_009680_1565 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 43.1 | -5.5 | -19.4 | 69.6 | 70.5 |
| Defrosting Dunes: PSP_009122_2600 PSP_009439_2600 (Interval in Earth days: 25) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.97 | 122. | 14.9 | -10.0 | 56.0 | 58.6 |
| Anatomy of a Well-Defined Crater Ray Emanating from Gratteri Crater: PSP_008514_1630 ESP_025445_1630 (Interval in Earth days: 1320) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.8 | 197. | -1.3 | -14.6 | 63.5 | 57.2 |
| Lobate Debris Apron with Ridge-Like Structures in Tempe Terra: PSP_009064_2315 PSP_009341_2315 (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 | 51.24 | 288. | 1.69 | -15.9 | 44.1 | 46.6 |
| Crater with Impressive Wind Streak in Elysium Planitia: PSP_008304_1860 ESP_012919_1860 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.728 | 169. | -2.0 | -11.4 | 49.1 | 55.9 |
| Basal Units in North Polar Region: PSP_009134_2645 PSP_009687_2645 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.66 | 157. | -7.5 | 10.32 | 60.3 | 62.1 |
| Zunil Crater Ray Formed within a Dusty Region: PSP_008225_1830 ESP_018510_1830 (Interval in Earth days: 801) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.916 | 167. | -2.7 | 16.38 | 50.1 | 51.7 |
| Crater in North Elysium Planitia As Seen in THEMIS Image V21264008: PSP_008807_2145 PSP_009796_2145 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.21 | 109. | 0.42 | -21.2 | 42.3 | 48.1 |
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