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.
| Central Pit of Large Crater South of Valles Marineris: PSP_007047_1640 PSP_010264_1640 (Interval in Earth days: 251) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.9 | 296. | -7.3 | 5.642 | 48.3 | 63.0 |
| Interior Channel in Durius Valles: PSP_007012_1630 PSP_007157_1630 (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 | -16.8 | 171. | -3.9 | 8.48 | 48.0 | 49.2 |
| Distal Rampart of Crater in Isidis Region: PSP_007740_1920 ESP_016047_1920 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.01 | 89.5 | -2.3 | 18.67 | 43.2 | 38.0 |
| Perplexing Landforms on Hellas Basin Floor: PSP_007135_1400 ESP_016088_1400 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 56.8 | -4.2 | 16.93 | 64.5 | 65.2 |
| Cones and Pitted Material Inside An Embayed Crater in the Tartarus Montes: PSP_007605_2055 PSP_007961_2055 (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 | 25.39 | 173. | 4.99 | -5.25 | 40.0 | 41.8 |
| Etched Terrain with Possible Layering West of Juventae Chasma: PSP_007482_1760 PSP_009486_1760 (Interval in Earth days: 156) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.20 | 296. | 1.06 | -9.01 | 47.0 | 58.5 |
| Central Peak of Large 40-Kilometer Diameter Crater: PSP_007592_1995 ESP_045595_1995 (Interval in Earth days: 2961) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.25 | 169. | -0.9 | 19.06 | 40.8 | 43.5 |
| Deposits in Kasei Valles: PSP_007970_2015 ESP_033551_2015 (Interval in Earth days: 1993) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.06 | 287. | -0.6 | 17.86 | 42.0 | 36.8 |
| Layering in Uzer Crater Wall Seen in MOC Image E01-00244: PSP_008073_1785 PSP_009721_1785 (Interval in Earth days: 128) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.27 | 358. | -2.0 | 13.86 | 51.2 | 55.4 |
| Gullies on South-Facing Wall of Crater: PSP_007045_1450 ESP_016130_1450 (Interval in Earth days: 708) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.6 | 353. | -5.7 | -23.5 | 59.8 | 64.8 |
Page 804 of 878 (8,772 images) | |||||