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.
| Fresh Crater: ESP_084505_1405 ESP_085217_1405 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.3 | 328. | 7.64 | -3.64 | 37.9 | 45.2 |
| Small Fresh Crater: ESP_084536_1160 ESP_085195_1160 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -63.8 | 208. | -2.9 | 29.34 | 52.6 | 59.7 |
| Yardangs near Scour Pit Field in Medusae Fossae Formation: ESP_084760_1730 ESP_085050_1730 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.94 | 200. | -2.4 | 19.25 | 36.3 | 33.6 |
| Gullied Crater Wall: ESP_084670_1435 ESP_085593_1435 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.9 | 142. | 2.83 | 23.40 | 37.7 | 47.0 |
| Streamlined Features in Hebrus Valles: ESP_084868_1995 ESP_085567_1995 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.18 | 127. | 9.06 | -7.83 | 47.5 | 42.1 |
| Small Fresh Crater: ESP_084518_1335 ESP_084874_1335 (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 | -46.0 | 335. | -3.9 | -20.3 | 41.8 | 45.9 |
| Channel with Streamlined Forms in Northeast Hellas Planitia: ESP_084725_1445 ESP_085635_1445 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.1 | 80.2 | 0 | -22.7 | 37.9 | 50.3 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084628_0935 ESP_084680_0935 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.3 | 250. | 3.97 | 18.69 | 70.7 | 70.3 |
| Cratered Cones in Amazonis Planitia: ESP_084866_2075 ESP_085011_2075 (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 | 27.42 | 182. | -3.2 | 6.99 | 53.9 | 51.4 |
| Valley in Newton Crater: ESP_084892_1375 ESP_085591_1375 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.3 | 201. | -4.8 | -16.4 | 43.0 | 53.6 |
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