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.
| Polar Layers Exposed on Promethei Lingula Surface: ESP_022139_0980 ESP_022258_0980 (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 | -81.7 | 112. | 8.35 | -8.06 | 60.2 | 61.6 |
| Manhattan Ice-Free Spider Terrain: ESP_022260_0935 ESP_022325_0935 (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 | -86.3 | 99.1 | -8.2 | 6.218 | 66.1 | 64.8 |
| Small Crater within Newton Crater with Gullies on Pole-Facing Slopes: ESP_022122_1400 ESP_021489_1405 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 203. | -15. | 1.708 | 39.2 | 45.7 |
| Possible Hematite-Rich Deposits along Crater Wall and Floor in Capri Chasma: ESP_022131_1665 ESP_022553_1665 (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 | -13.2 | 312. | 0 | -15.0 | 39.9 | 36.3 |
| Gale Crater Rim Deposits: ESP_022045_1745 ESP_022190_1745 (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 | -5.43 | 138. | 4.26 | 18.22 | 43.9 | 41.2 |
| Possible MSL Rover Landing and Seismic Network Site in Utopia Region: ESP_022178_1960 ESP_022534_1960 (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 | 15.61 | 105. | -3.8 | 4.541 | 55.5 | 50.9 |
| Stereo of Seasonal/Yearly SPRC Monitoring Site: ESP_022197_0935 ESP_022592_0935 (Interval in Earth days: 30) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.3 | 3.59 | -1.9 | 8.738 | 65.0 | 66.4 |
| Faults in the South Polar Layered Deposits: ESP_022126_0995 ESP_022100_0995 (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 | -80.2 | 100. | 18.8 | -2.52 | 58.5 | 59.9 |
| Possible Future Mars Landing Site with Inverted River Meanders: ESP_022084_1740 ESP_022361_1740 (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 | -5.72 | 153. | 12.8 | -21.6 | 42.7 | 41.8 |
| Channel Fill and Sinuous Ridge Material Southwest of Capen Crater: ESP_022221_1850 ESP_039667_1850 (Interval in Earth days: 1360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.959 | 12.6 | 0.78 | -15.1 | 47.8 | 52.8 |
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