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.
| Light-Toned Blocks in or on Melas Chasma Landslide Deposit: ESP_022844_1680 ESP_031112_1680 (Interval in Earth days: 644) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.9 | 285. | 2.34 | -25.2 | 32.8 | 40.5 |
| Clustered Mounds in Hypanis Valles Region: ESP_023001_1925 ESP_023278_1925 (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 | 12.31 | 316. | 4.36 | -18.6 | 42.7 | 41.1 |
| Anastomosing Slope Lineae: ESP_023020_1900 ESP_023297_1900 (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 | 9.947 | 157. | 2.53 | -20.1 | 41.1 | 39.8 |
| The Crazy Floor of the Hellas Basin: ESP_023234_1460 ESP_024091_1460 (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 | -33.5 | 81.5 | 0.57 | 28.11 | 36.3 | 46.4 |
| Starburst Spiders at a South Polar Cracked and Gullied Site: ESP_023117_0980 ESP_022998_0980 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.6 | 66.2 | -18. | -2.77 | 70.6 | 67.8 |
| Fan-Shaped Deposit in a Valles Marineris Trough: ESP_022949_1650 ESP_030518_1650 (Interval in Earth days: 590) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 299. | -1.6 | 21.10 | 32.0 | 42.9 |
| Light-Toned Material along Valley near Coprates Catena: ESP_022527_1645 ESP_023028_1645 (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 | -15.5 | 300. | 1.62 | 23.37 | 34.6 | 29.7 |
| Eastern Half of Iazu Crater: ESP_022670_1775 ESP_023092_1775 (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 | -2.69 | 354. | 8.00 | -9.77 | 37.6 | 34.9 |
| Central Uplift of Impact Crater: ESP_022454_1470 ESP_022599_1470 (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 | -32.5 | 136. | -0.5 | 16.53 | 34.4 | 32.5 |
| Stratigraphy of Kasimov Crater Fill: ESP_022473_1550 ESP_023119_1550 (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 | -24.9 | 337. | -8.5 | 27.5 | 34.5 | 30.2 |
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