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.
| Landslide Facing West near Cydonia Mensae: ESP_080456_2115 ESP_080522_2115 (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 | 31.37 | 347. | 12.1 | -5.83 | 47.5 | 49.5 |
| Curvilinear Ridges on Floor of Shalbatana Vallis: ESP_080589_1885 ESP_080233_1885 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.367 | 318. | 19.4 | -1.16 | 52.6 | 53.6 |
| Juventae Chasma Interior Deposit Layers: ESP_080458_1755 ESP_080669_1755 (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 | -4.62 | 297. | 11.5 | -0.14 | 58.9 | 59.5 |
| Grooves and Cataracts in Eos Chasma: ESP_080576_1665 ESP_080431_1665 (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 | -13.3 | 318. | -0.6 | -16.6 | 64.1 | 65.6 |
| Dunes near Syrtis Major Planum Crater Ejecta: ESP_080242_1970 ESP_080308_1970 (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 | 16.58 | 72.6 | -8.3 | -24.6 | 51.1 | 52.7 |
| Streamlined Features in Athabasca Valles: ESP_080595_1890 ESP_080740_1890 (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 | 8.663 | 156. | 6.28 | 17.47 | 53.5 | 52.9 |
| Eroded Sedimentary Rock Layers: ESP_080568_1670 ESP_080779_1670 (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 | -12.7 | 176. | -1.1 | -14.0 | 63.8 | 64.2 |
| A Fissure Vent East of Olympus Mons: ESP_080579_1955 ESP_080790_1955 (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 | 15.48 | 232. | 5.92 | -6.42 | 51.4 | 53.1 |
| Crustal Blocks in the Walls of Coprates Chasma: ESP_080616_1640 ESP_078282_1640 (Interval in Earth days: 181) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 304. | 22.8 | -1.64 | 63.6 | 58.0 |
| Defrosting Dunes in Chasma Boreale: ESP_080112_2645 ESP_080139_2645 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.55 | 336. | 8.30 | -5.70 | 61.4 | 62.2 |
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