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.
| Jezero Crater: ESP_094047_1985 ESP_093981_1985 (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 | 18.47 | 77.4 | -7.4 | 15.88 | 43.8 | 42.9 |
| South Polar Layering: ESP_093824_0990 ESP_093877_0990 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.0 | 71.1 | 0.96 | -13.3 | 71.8 | 73.6 |
| Irregular Cellular Structures around Crater in Arabia Terra: ESP_094101_2145 ESP_093165_2145 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.03 | 39.6 | 5.77 | -18.1 | 52.4 | 66.3 |
| Margin of Smooth Deposit East of Argyre Planitia: ESP_094038_1340 ESP_094117_1340 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.5 | 331. | -5.7 | 21.06 | 49.0 | 48.6 |
| McMurdo Crater Layers: ESP_093919_0955 ESP_094024_0955 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.5 | 0.54 | 9.95 | 24.47 | 75.7 | 76.6 |
| Shalbatana Vallis Degraded Channel Floor Material: ESP_093801_1840 ESP_092878_1840 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.187 | 315. | -4.2 | 19.21 | 38.5 | 46.7 |
| Possible Landing Site for Mars Rotorcraft: ESP_094122_2190 ESP_090694_2190 (Interval in Earth days: 267) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.53 | 187. | -9.1 | -0.97 | 56.2 | 63.9 |
| Inverted Channel in Noachis Terra: ESP_094129_1455 ESP_093338_1455 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.3 | 4.54 | 0.48 | -10.0 | 43.2 | 37.1 |
| Ares Vallis: ESP_093840_1945 ESP_085731_1945 (Interval in Earth days: 632) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.43 | 331. | -19. | 5.715 | 44.4 | 38.7 |
| Irregular Cellular Structures around Crater in Southern Mid-Latitudes: ESP_094116_1400 ESP_093549_1400 (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 | -39.4 | 1.17 | -8.9 | 16.40 | 46.6 | 38.3 |
Page 1 of 906 (9,054 images) | |||||