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.
| Potential Chloride-Rich Deposit near Mawrth Vallis: ESP_089739_2065 ESP_089884_2065 (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 | 26.05 | 340. | 8.34 | 23.47 | 50.2 | 50.0 |
| Iani Chaos: ESP_089660_1780 ESP_089238_1780 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.75 | 341. | -6.6 | 6.11 | 57.5 | 56.6 |
| Fretted Terrain Valley Head in Coloe Fossae: ESP_089723_2160 ESP_090290_2160 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.80 | 56.1 | 2.51 | 18.35 | 50.9 | 56.0 |
| Inverted Valley and Rings in Erebus Montes: ESP_089718_2210 ESP_090061_2210 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.86 | 188. | 26.6 | -1.13 | 49.3 | 55.9 |
| Moraine-Like Assemblage Exposed by Ice Retreat: ESP_089855_2215 ESP_090422_2215 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.98 | 51.3 | 6.63 | 23.73 | 52.7 | 58.7 |
| Antoniadi Crater Fluvial Features: ESP_089868_2015 ESP_089934_2015 (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 | 21.20 | 57.4 | 26.6 | 9.6 | 49.7 | 51.7 |
| Large Alluvial Fan in Kasei Valles: ESP_089846_2065 ESP_089991_2065 (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 | 26.23 | 300. | -2.1 | 14.95 | 51.9 | 51.7 |
| Barchan to Sand Sheet Transition in Central Herschel Crater: ESP_089892_1655 ESP_090037_1655 (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 | -14.1 | 129. | -3.4 | 17.28 | 62.1 | 60.1 |
| Closed Fretted Terrain Valley: ESP_089724_2185 ESP_089790_2185 (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 | 38.34 | 28.0 | 6.60 | -9.01 | 50.9 | 52.9 |
| Crater Exposing Layers in Icy Deposits: ESP_089851_2175 ESP_090128_2175 (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 | 36.92 | 161. | 8.87 | -6.46 | 51.8 | 56.4 |
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