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.
| Interior of Western Candor Chasma: PSP_003474_1735 PSP_003540_1735 (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 | -6.44 | 283. | 17.0 | -6.73 | 51.8 | 53.2 |
| Light-toned Layering along Plains and in Pit floor Next to Juventae Chasma: PSP_004990_1755 ESP_012255_1755 (Interval in Earth days: 566) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.64 | 296. | -3.4 | 23.55 | 39.1 | 53.5 |
| Depositional Fan : PSP_002387_1985 PSP_003798_1985 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.48 | 77.4 | 1.71 | -15.8 | 55.6 | 63.7 |
| Proposed MSL Site in Meridiani Crater: PSP_002179_1855 ESP_063535_1855 (Interval in Earth days: 4781) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.421 | 358. | -3.6 | 18.24 | 54.7 | 52.5 |
| Crater in Western Arabia Terra with Stair-Stepped Hills and Dark Dunes: PSP_001902_1890 PSP_002047_1890 (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 | 8.814 | -1.0 | 11.6 | 25.47 | 52.0 | 51.3 |
| Southern Layered Mound and Floor in Gale Crater: PSP_002464_1745 PSP_003176_1745 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.51 | 138. | 2.93 | 21.29 | 55.7 | 52.8 |
| Inverted Channels near Juventae Chasma: PSP_003223_1755 PSP_003724_1755 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.31 | 296. | 0 | 27.52 | 54.6 | 50.0 |
| MSL Landing Site in Melas Chasma: PSP_002828_1700 ESP_019508_1700 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.82 | 283. | -28. | -5.16 | 58.0 | 58.0 |
| Putative Polyhydrated Sulfate Deposits in East Melas Chasma: PSP_003487_1670 ESP_040936_1670 (Interval in Earth days: 2918) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.6 | 290. | 0 | -25.0 | 51.7 | 35.6 |
| Proposed Strandline: PSP_001820_1985 PSP_003442_1985 (Interval in Earth days: 126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.25 | 77.3 | 1.02 | -22.9 | 51.3 | 64.1 |
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