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.
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_078674_2295 ESP_078595_2295 (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 | 49.27 | 30.2 | 16.0 | -5.49 | 43.8 | 45.8 |
| Large Phyllosilicate Deposit near Magelhaens Crater: ESP_078827_1485 ESP_080449_1485 (Interval in Earth days: 126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.9 | 185. | 2.50 | 18.61 | 73.0 | 73.9 |
| Bedrock in Northeast Syrtis Major Region: ESP_078712_1980 ESP_087494_1975 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.48 | 77.2 | 26.2 | -10.1 | 43.1 | 45.3 |
| Well-Preserved 9-Kilometer Impact Crater: ESP_078821_1740 ESP_079243_1740 (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 | -5.81 | 346. | 5.18 | -7.41 | 56.3 | 59.3 |
| Pedestal Crater: ESP_078706_2485 ESP_078838_2485 (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 | 68.14 | 231. | 8.43 | -6.71 | 52.1 | 52.6 |
| Bright and Round Deposit in Eos Chasma: ESP_078888_1665 ESP_079244_1665 (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 | -13.1 | 319. | -8.5 | 2.452 | 62.1 | 63.3 |
| Partial Icy Fill of Impact Crater onto Graben: ESP_078679_2170 ESP_078824_2170 (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 | 36.46 | 258. | -6.1 | 5.368 | 43.4 | 42.5 |
| Crater in Oxia Planum: ESP_078650_1965 ESP_079151_1965 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.43 | 333. | -9.7 | 12.74 | 46.2 | 46.4 |
| Sedimentary Layers in Hebes Chasma: ESP_078942_1795 ESP_079298_1795 (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 | -0.55 | 282. | 4.64 | 16.17 | 54.0 | 54.8 |
| Terrain Sample near Jezero Crater: ESP_078844_1980 ESP_078989_1980 (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 | 17.61 | 76.4 | -6.5 | 8.294 | 46.4 | 45.7 |
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