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.
| Gullies in Dao Valles: PSP_001635_1445 PSP_001978_1445 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.3 | 91.1 | 4.16 | -5.48 | 72.2 | 69.9 |
| Irregular Structures in Huo Hsing Vallis: PSP_002150_2110 PSP_002282_2110 (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 | 30.77 | 65.4 | 8.03 | -27.0 | 54.7 | 59.4 |
| Cataracts in Kasei Valles : PSP_002814_2055 PSP_003513_2055 (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 | 25.07 | 298. | 4.29 | -26.3 | 60.9 | 68.0 |
| Chasma Boreale Scarp with Possible Gypsum: PSP_001374_2650 PSP_001518_2650 (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 | 85.02 | 338. | -7.1 | 13.56 | 67.9 | 68.9 |
| Lineated Valley Fill in Coloe Fossae : PSP_002902_2205 PSP_003245_2205 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.17 | 53.8 | 3.42 | -28.6 | 68.2 | 74.8 |
| 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 | 65.7 | 68.7 |
| Fresh Impact Crater with Bright, Rocky Ejecta: PSP_001782_1655 PSP_002204_1655 (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 | -14.1 | 38.6 | 2.21 | -11.5 | 60.1 | 59.5 |
| Tomini Crater, Rayed: PSP_001871_1965 ESP_024419_1965 (Interval in Earth days: 1757) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.25 | 125. | -6.9 | -19.7 | 52.5 | 38.0 |
| Eroded Layers and Scallops and Polygons: PSP_001964_2275 PSP_003177_2275 (Interval in Earth days: 95) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.94 | 101. | -0.2 | 25.63 | 57.4 | 73.4 |
| 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 |
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