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.
| Escarpment Dune Field Topography: ESP_088713_2640 ESP_088819_2640 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.92 | 233. | 8.93 | -5.01 | 59.8 | 60.9 |
| Contact between Crater and Flood Lava: ESP_088744_1845 ESP_089034_1845 (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 | 4.224 | 148. | 3.14 | 26.44 | 53.6 | 52.0 |
| Flow Entering Fretted Terrain Valley: ESP_088735_2170 ESP_088669_2170 (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 | 36.59 | 32.1 | -14. | 4.335 | 45.7 | 43.8 |
| Wavy Terrain: ESP_088677_1725 ESP_088743_1725 (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 | -7.35 | 179. | 4.11 | -20.5 | 59.9 | 61.6 |
| Aeolis Dorsa Inverted Deposits: ESP_088612_1735 ESP_088823_1735 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.35 | 154. | -1.4 | -14.9 | 59.6 | 60.6 |
| Canyon Walls in Coprates Chasma: ESP_088646_1655 ESP_088857_1655 (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 | -14.1 | 306. | 4.01 | -9.22 | 64.2 | 64.9 |
| Platy-Ridged Lava: ESP_088635_2000 ESP_088780_2000 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.88 | 243. | -1.4 | 9.447 | 47.2 | 46.7 |
| Dune Monitoring near Utopia Rupes: ESP_088746_2270 ESP_089036_2270 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.72 | 88.9 | -3.2 | 12.36 | 45.4 | 45.6 |
| Channels along Hydraotes Chaos Channel: ESP_088566_1835 ESP_088711_1835 (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 | 3.377 | 329. | 3.41 | 14.35 | 53.8 | 53.2 |
| Steep Sandy Slopes in Coprates Chasma: ESP_088554_1660 ESP_088620_1660 (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 | -13.7 | 298. | 11.2 | -14.2 | 63.4 | 65.0 |
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