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.
| Middle Section of Northern Olympus Mons Basal Scarp: PSP_007089_2035 PSP_007946_2035 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.25 | 223. | 7.43 | -6.64 | 38.8 | 42.1 |
| Line of Cones and Associated Flows in Arsia Sulci: PSP_007603_1770 ESP_036718_1770 (Interval in Earth days: 2269) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.83 | 231. | 8.18 | -17.6 | 47.1 | 57.8 |
| Complex Layered Deposits in Tithonium Chasma: PSP_007918_1755 PSP_008274_1755 (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 | -4.64 | 270. | 6.16 | -5.59 | 51.1 | 54.6 |
| Large Dunes Possibly of Aqueous Origin in Gale Crater: PSP_007356_1750 PSP_008147_1750 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.19 | 137. | -4.1 | 6.367 | 46.5 | 53.3 |
| Blocky Deposit and Valley Networks Along Melas Chasma Wallrock: PSP_007443_1705 PSP_007733_1705 (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 | -9.17 | 282. | -9.1 | 5.346 | 49.8 | 52.0 |
| Eroded Craters on the Medusae Fossae Formation: PSP_008186_1840 PSP_009267_1840 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.049 | 152. | -4.4 | 16.56 | 49.4 | 52.0 |
| Lineated Valley Fill in Deuteronilus Mensae: PSP_007795_2175 PSP_009588_2175 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.35 | 24.6 | -4.2 | 7.505 | 42.0 | 44.3 |
| Libya Montes Hydrated Minerals: PSP_007503_1840 ESP_024526_1840 (Interval in Earth days: 1326) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.763 | 82.2 | -3.4 | 22.04 | 44.2 | 35.1 |
| Fault Relays in the Cerberus Fossae: PSP_007645_1885 PSP_007856_1885 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.465 | 164. | -5.5 | -23.3 | 43.9 | 46.8 |
| Gullies and Bedrock Exposures in Impact Crater Wall: PSP_008153_1480 PSP_009155_1480 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.4 | 337. | 4.51 | -12.3 | 70.8 | 76.3 |
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