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.
| InSight Mission Candidate Landing Site: ESP_036484_1835 ESP_037051_1835 (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 | 3.321 | 137. | 8.92 | -5.29 | 53.1 | 55.1 |
| Small Crater in Utopia Planitia: ESP_036446_2250 ESP_037224_2250 (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 | 44.61 | 90.6 | -3.2 | -17.2 | 48.2 | 58.5 |
| Crater Cluster on North Polar Layered Deposits: ESP_036608_2620 ESP_036423_2620 (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 | 81.83 | 333. | -7.0 | 8.635 | 65.5 | 62.6 |
| Steep North Polar Peripheral Scarp: ESP_036548_2655 ESP_036799_2655 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.23 | 160. | -6.8 | -17.2 | 66.9 | 70.6 |
| Very Fresh Small Crater: ESP_036685_1670 ESP_037397_1670 (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 | -12.8 | 52.7 | -4.1 | 7.672 | 61.6 | 58.8 |
| Landforms Near Nili Fossae: ESP_036552_2000 ESP_036763_2000 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.67 | 78.9 | 8.38 | -4.42 | 48.2 | 50.4 |
| Head of Jezero Crater Fan: ESP_036618_1985 ESP_037119_1985 (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 | 18.51 | 77.2 | 5.83 | 17.35 | 49.0 | 51.0 |
| Channels Near Contact Between Chryse Planitia and Vistula Valles: ESP_036715_1945 ESP_037348_1945 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.31 | 309. | 7.04 | -18.6 | 50.3 | 55.9 |
| Korolev Crater Changes: ESP_036654_2530 ESP_036852_2530 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 72.79 | 164. | -4.5 | -22.0 | 60.9 | 65.0 |
| Light-Toned Deposits with Possible Inverted Channels in Eridani Region: ESP_036509_1485 ESP_052768_1485 (Interval in Earth days: 1267) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.1 | 180. | -0.0 | -18.7 | 72.6 | 72.9 |
Page 463 of 896 (8,955 images) | |||||