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.
| Relatively Pristine 7-Kilometer Crater with Gullies: ESP_066597_1435 ESP_066465_1435 (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 | -36.3 | 302. | 1.02 | 24.41 | 39.4 | 37.9 |
| Scarp Fronted Deposit in South Gunjur Crater: ESP_066774_1795 ESP_067526_1795 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.32 | 146. | 8.48 | 17.64 | 43.5 | 38.5 |
| Central Deposit and Possible Exit Breach: ESP_066805_1440 ESP_067557_1440 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 25.9 | 1.63 | 11.85 | 39.1 | 44.5 |
| Layered Deposits within Depression in Osuga Valles: ESP_066583_1650 ESP_065897_1650 (Interval in Earth days: 53) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.8 | 322. | -10. | 10.02 | 41.2 | 46.6 |
| South Polar Layered Deposits: ESP_066784_0915 ESP_067023_0915 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.3 | 284. | 21.7 | 14.13 | 68.7 | 72.9 |
| Oyama Crater: ESP_066780_2040 ESP_066991_2040 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.79 | 340. | -1.6 | 21.25 | 58.6 | 54.7 |
| Features in Mamers Valles: ESP_066528_2215 ESP_075391_2215 (Interval in Earth days: 690) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.30 | 14.3 | 5.69 | -4.18 | 74.0 | 73.2 |
| Clay-Rich Stratigraphy South of Coprates Chasma: ESP_066531_1650 ESP_067626_1650 (Interval in Earth days: 85) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 301. | -8.7 | 5.387 | 41.4 | 39.1 |
| Craters with Steep Slopes: ESP_066516_1445 ESP_084570_1445 (Interval in Earth days: 1407) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.1 | 352. | 1.33 | 7.927 | 39.4 | 36.6 |
| Candidate Recent Impact Site: ESP_066587_2040 ESP_067062_2040 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.57 | 206. | 6.35 | -14.7 | 60.3 | 55.8 |
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