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.
| Valleys in Crater Northeast of Argyre Region: ESP_067704_1500 ESP_073784_1500 (Interval in Earth days: 474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.6 | 334. | 7.13 | 20.86 | 44.0 | 53.7 |
| Inverted Channel in Cusus Valles: ESP_067833_1960 ESP_067965_1960 (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 | 16.05 | 49.8 | 5.88 | -3.77 | 43.8 | 44.2 |
| Mounds in Acidalia Planitia: ESP_068074_2280 ESP_068483_2280 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.47 | 312. | -7.6 | 26.38 | 59.5 | 53.0 |
| Two Notches near Lowest Elevation Point of Crater Rim: ESP_067821_1465 ESP_067689_1465 (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 | -33.2 | 24.7 | -7.3 | 6.887 | 48.4 | 45.5 |
| Gullies Eroding Thick Mantling Deposits: ESP_067903_1370 ESP_073574_1370 (Interval in Earth days: 442) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.6 | 308. | -5.4 | 22.27 | 54.7 | 59.3 |
| Terrain in Cydonia Region: ESP_067848_2205 ESP_068970_2200 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.15 | 358. | -1.9 | -16.2 | 57.0 | 50.7 |
| Landforms on Floor of Wahoo Crater: ESP_067902_2040 ESP_067493_2040 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.50 | 326. | 8.19 | -6.89 | 46.5 | 50.7 |
| Eroded Crater with Eroded Floor in Hellas Region: ESP_067435_1385 ESP_076680_1385 (Interval in Earth days: 721) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.9 | 116. | -2.8 | 6.995 | 46.5 | 49.9 |
| Crater near Uranius Mons: ESP_067495_2080 ESP_067363_2080 (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 | 27.80 | 271. | -7.2 | 8.657 | 53.2 | 53.7 |
| Small Impact Crater Exposed by Erosion: ESP_067455_1755 ESP_067930_1755 (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 | -4.48 | 286. | -3.2 | 8.213 | 39.3 | 40.2 |
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