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 Deposits along Channel: ESP_093100_1335 ESP_093245_1335 (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 | -46.0 | 22.9 | 0.12 | 12.69 | 40.4 | 39.9 |
| Possible Compound Dune in USGS Dune Database Entry Number 0349-763: ESP_093166_1035 ESP_092968_1035 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -76.3 | 34.9 | -10. | 7.706 | 60.2 | 57.7 |
| Chryse Chaos: ESP_093102_1935 ESP_093392_1935 (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 | 13.33 | 322. | -17. | 16.34 | 52.1 | 46.4 |
| Constrain Juventae Chasma Interior Deposit Layer Orientations: ESP_093393_1765 ESP_093037_1765 (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 | -3.33 | 298. | -2.1 | -14.6 | 38.4 | 43.0 |
| Alluvial Fan in Melas Chasma: ESP_093446_1665 ESP_093301_1665 (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 | -13.4 | 289. | 29.6 | 16.15 | 32.3 | 34.5 |
| Gully with Small Alcove in Southern Mid-Latitude Crater: ESP_093397_1335 ESP_093265_1335 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.2 | 196. | -17. | 13.37 | 42.9 | 40.0 |
| Stereo for Partially Eroded Dunes in Southern Terra Cimmeria: ESP_093214_1150 ESP_093082_1150 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -64.8 | 154. | 2.74 | 22.91 | 51.5 | 49.4 |
| Dark Sand Deposits on Sharp and Rounded Dune Crests in Noachis Terra: ESP_093351_1185 ESP_093061_1185 (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 | -61.0 | 14.6 | -6.0 | -22.7 | 50.7 | 49.8 |
| Landforms Above Subsurface Radar Observations of South Polar Cap: ESP_093175_1025 ESP_084802_1025 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.2 | 153. | -19. | -9.68 | 61.6 | 66.2 |
| Arcing Ridge in Meridiani Planum: ESP_093312_1870 ESP_093246_1870 (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 | 6.776 | 347. | 11.4 | 29.84 | 43.6 | 43.0 |
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