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.
| Banded or Terraced Hillslopes in East Hellas Planitia : ESP_052231_1410 ESP_060974_1410 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.5 | 82.4 | -4.9 | 20.53 | 74.5 | 73.0 |
| Lava Contacts in Elysium Planitia Region : ESP_052333_1895 ESP_052478_1895 (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 | 9.593 | 170. | 4.96 | 15.14 | 43.3 | 43.2 |
| Fan Material at an Alcove on Southwestern Aeolis Mons : ESP_052242_1745 ESP_063319_1745 (Interval in Earth days: 863) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.48 | 137. | -1.7 | 14.83 | 51.1 | 56.0 |
| Large Slope Streaks : ESP_052293_1955 ESP_052583_1955 (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 | 15.10 | 181. | 7.51 | 26.00 | 40.7 | 40.3 |
| Twin Channels in Innsbruck Crater : ESP_052143_1735 ESP_052565_1735 (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 | -6.49 | 320. | -0.5 | -26.3 | 50.9 | 55.5 |
| Chains of Mounds in Utopia Planitia : ESP_052283_2075 ESP_052718_2075 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.04 | 94.1 | -5.7 | 21.52 | 39.1 | 37.7 |
| Possible Inverted Channel within Valley : ESP_052082_1680 ESP_052227_1680 (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 | -11.7 | 185. | 3.53 | 19.32 | 53.4 | 53.6 |
| Unusual Hills West of Olympus Mons : ESP_052015_1950 ESP_052160_1950 (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 | 14.88 | 211. | 3.55 | 20.46 | 39.7 | 39.1 |
| Channel and Flow That Cut Crater Rim and Wall in Daedalia Planum : ESP_052357_1570 ESP_052568_1570 (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 | -22.8 | 239. | 2.19 | -12.0 | 63.4 | 65.5 |
| Candidate Red Dragon Landing Site in Arcadia Planitia : ESP_052358_2210 ESP_052134_2210 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.71 | 201. | 17.9 | -15.0 | 37.6 | 40.8 |
Page 311 of 878 (8,777 images) | |||||