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.
| 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 |
| Features around Crater in Terra Sabaea: ESP_089842_2165 ESP_089565_2165 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.09 | 50.5 | -24. | -6.66 | 54.5 | 50.2 |
| 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 |
| 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 |
| Scarp Contact: ESP_089889_1920 ESP_090166_1920 (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 | 11.85 | 207. | 1.64 | -17.1 | 53.2 | 56.1 |
| Streamlined Shape and Possible Bar South of Semeykin Crater: ESP_089883_2195 ESP_090028_2195 (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 | 39.01 | 8.16 | -0.2 | 14.06 | 53.3 | 53.8 |
| Exposed Layers in Olympia Mensae Icy Outliers: ESP_089774_2545 ESP_089787_2545 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.13 | 95.1 | -4.3 | 10.35 | 64.8 | 63.9 |
| 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 |
| Kasei Valles Alluvial Fan and Distributary Channels: ESP_089899_2035 ESP_089622_2035 (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 | 23.09 | 293. | -4.0 | 17.28 | 52.5 | 48.8 |
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