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.
| Elysium Mons Caldera: ESP_035811_2050 ESP_037011_2050 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.62 | 146. | 9.77 | -1.00 | 44.1 | 51.6 |
| Terraced Mesas in Mamers Valles: ESP_035697_2195 ESP_035763_2195 (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 | 39.24 | 16.8 | 8.52 | -7.04 | 42.1 | 43.7 |
| Possible Chlorite-Bearing Knob in Northwest Hellas Region: ESP_035656_1530 ESP_035801_1530 (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 | -26.8 | 66.3 | -7.3 | 10.43 | 72.3 | 71.2 |
| Equatorial Gullies on Mars: ESP_035945_1755 ESP_036433_1755 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.50 | 92.6 | 7.48 | -11.1 | 57.0 | 58.2 |
| A Heart in Ascraeus Mons: ESP_035807_1885 ESP_036862_1885 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.176 | 258. | 9.65 | -14.9 | 50.0 | 54.0 |
| Slumping Terraces on a Crater Wall : ESP_035702_2270 ESP_035768_2270 (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 | 46.54 | 238. | 8.98 | -4.85 | 42.7 | 44.2 |
| Ring of Cratered Cones: ESP_035098_2065 ESP_034808_2065 (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 | 26.23 | 170. | 22.2 | 0 | 40.4 | 41.6 |
| Mission 2020: A Candidate Landing Site in Gusev Crater: ESP_035164_1655 ESP_036087_1655 (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 | -14.5 | 175. | 6.33 | 27.49 | 61.9 | 61.5 |
| Sediment Routing System in Aeolis Dorsa: ESP_035455_1780 ESP_036800_1780 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.78 | 149. | 4.58 | 17.96 | 54.9 | 54.7 |
| Erosional Morphologies in Outflow Channel Bend of Shalbatana Vallis: ESP_035396_1890 ESP_037097_1890 (Interval in Earth days: 133) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.680 | 319. | 4.05 | 19.88 | 49.2 | 51.9 |
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