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 Deposits along Melas Chasma Floor: ESP_025178_1705 ESP_025244_1705 (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 | -9.57 | 283. | 12.5 | -10.2 | 48.1 | 50.4 |
| Light-Toned Material and Dark Dunes and Gullies: ESP_025177_2145 ESP_026245_2145 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.12 | 306. | 2.29 | 29.34 | 39.6 | 37.3 |
| Floor of Toro Crater: ESP_025344_1970 ESP_025067_1970 (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 | 17.00 | 71.7 | -24. | 0.616 | 41.9 | 38.4 |
| Daedalia Planum Reticulate Bedform Changes: ESP_025233_1610 ESP_025088_1610 (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 | -18.6 | 223. | 13.9 | -2.92 | 54.3 | 53.5 |
| Possible Phyllosilicates Northwest of Hellas Region: ESP_025107_1535 ESP_034232_1535 (Interval in Earth days: 711) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.2 | 64.5 | 7.13 | -6.50 | 58.2 | 63.5 |
| Slope Streaks in Pettit Crater: ESP_025287_1920 ESP_025643_1925 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.20 | 186. | 0 | 14.88 | 40.5 | 41.5 |
| Fresh Crater on Northern Plains: ESP_025366_2305 ESP_025498_2305 (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 | 50.19 | 184. | -3.4 | -26.3 | 45.0 | 46.4 |
| Pitted Central Uplift: ESP_025069_2250 ESP_025135_2250 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.67 | 12.7 | 4.58 | -10.1 | 43.4 | 44.3 |
| Changes in Intracrater Dunes: ESP_025144_1420 ESP_024854_1420 (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 | -37.7 | 136. | 0.92 | -24.0 | 67.3 | 64.7 |
| Arabia Terra Bedforms: ESP_025267_1795 ESP_024990_1795 (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 | -0.35 | 15.0 | -15. | 13.24 | 46.3 | 41.4 |
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