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.
| Bright Gully Deposits in Hale Crater: PSP_006822_1440 PSP_007468_1440 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 322. | -6.4 | 4.941 | 57.0 | 66.1 |
| Gullies with Dark Channels on South-Facing Crater Slope: PSP_005194_1445 PSP_005471_1445 (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 | -35.0 | 130. | -2.9 | -27.7 | 35.7 | 39.1 |
| Bright Layers in Columbus Crater: PSP_005429_1510 PSP_005851_1510 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.4 | 193. | -4.6 | -17.2 | 34.6 | 38.9 |
| Erosional Features and Knob in Argyre Planitia: PSP_005860_1340 ESP_011424_1340 (Interval in Earth days: 433) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.4 | 308. | 3.54 | 17.72 | 47.2 | 66.8 |
| Ancient Valley Network Adjacent to Low-Albedo Outcrops: PSP_004832_1310 PSP_005465_1310 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.6 | 294. | 6.60 | -9.99 | 40.0 | 44.9 |
| Complex Banded Terrain of Hellas Floor: PSP_006555_1395 PSP_007122_1395 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.1 | 52.6 | 0 | -11.5 | 55.2 | 65.2 |
| Apparent Fluvial Channel at the Summit of Hecates Tholus: PSP_004982_2120 PSP_005259_2120 (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 | 31.70 | 150. | -3.6 | -27.4 | 63.0 | 60.7 |
| Layering in Graben Wall: PSP_005902_2265 ESP_085761_2265 (Interval in Earth days: 6222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.97 | 229. | 3.76 | -10.1 | 60.9 | 56.0 |
| Eridania Scopulus: PSP_006565_1270 ESP_011338_1270 (Interval in Earth days: 372) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.7 | 141. | 0 | -12.7 | 64.5 | 73.4 |
| Impact Flow Features: PSP_005616_1440 ESP_011536_1440 (Interval in Earth days: 461) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 129. | -4.5 | 21.05 | 38.9 | 61.4 |
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