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.
| Anastomosing Slope Lineae: ESP_023020_1900 ESP_023297_1900 (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 | 9.947 | 157. | 2.53 | -20.1 | 41.1 | 39.8 |
| Impact Crater on Polar Layered Deposits: ESP_022944_0920 ESP_023048_0920 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 133. | 16.5 | 28.10 | 71.9 | 72.1 |
| Proposed Landing Site in Nili Fossae: ESP_022878_2010 ESP_022812_2010 (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 | 20.69 | 74.5 | -10. | 11.12 | 50.9 | 50.6 |
| Northern Floor of Oudemans Crater: ESP_022871_1705 ESP_023148_1705 (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 | -9.48 | 268. | 4.85 | -23.5 | 33.2 | 33.9 |
| Light-Toned Material, Possibly Opal, in Noctis Trough: ESP_023003_1710 ESP_023359_1710 (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 | -9.07 | 264. | 6.08 | 22.16 | 32.3 | 29.9 |
| Fresh 2-Kilometer Crater: ESP_022924_1405 ESP_023201_1405 (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 | -39.1 | 264. | 5.18 | -17.5 | 36.2 | 40.0 |
| Barchan to Linear to Transverse Dune Transition in Summer: ESP_022775_1205 ESP_023065_1205 (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 | -58.9 | 16.8 | 1.70 | 18.55 | 47.2 | 49.3 |
| Possible Olivine-Rich Crater in Terra Sirenum: ESP_022952_1305 ESP_050327_1305 (Interval in Earth days: 2133) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.3 | 223. | -5.1 | 22.16 | 42.8 | 54.0 |
| Well Exposed Layered Deposits and Possible MSL Rover Landing Site: ESP_022707_1505 ESP_022562_1505 (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 | -29.0 | 67.6 | 11.1 | -3.05 | 32.0 | 33.6 |
| Fan at Intersection of Valley and Depression Floor: ESP_023036_1310 ESP_023313_1310 (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 | -48.6 | 88.3 | 8.17 | -8.33 | 42.4 | 46.8 |
Page 601 of 866 (8,658 images) | |||||