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.
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088500_2435 ESP_088421_2435 (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 | 62.98 | 320. | 7.80 | -6.45 | 48.1 | 49.1 |
| Kasei Valles Alluvial Fans: ESP_088633_2040 ESP_088778_2040 (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 | 23.55 | 298 | -6.4 | 3.817 | 46.5 | 46.1 |
| North Polar Layered Deposits Structural Geology in Icy Layers: ESP_088733_2630 ESP_088562_2630 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.71 | 56.5 | 6.65 | -7.41 | 59.1 | 59.3 |
| Aeolis Dorsa Inverted Deposits: ESP_088612_1735 ESP_088823_1735 (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 | -6.35 | 154. | -1.4 | -14.9 | 59.6 | 60.6 |
| Channels along Hydraotes Chaos Channel: ESP_088566_1835 ESP_088711_1835 (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 | 3.377 | 329. | 3.41 | 14.35 | 53.8 | 53.2 |
| Fan-Shaped Feature in Ismenius Lacus: ESP_088485_2145 ESP_088696_2145 (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 | 33.95 | 17.5 | -4.9 | -15.7 | 44.2 | 45.9 |
| Crater and Flow in Daedalia Planum: ESP_088557_1685 ESP_089058_1685 (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 | -11.5 | 217. | -8.9 | 3.217 | 63.3 | 62.3 |
| Layering and Contact in Lucus Planum: ESP_088545_1725 ESP_088756_1725 (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 | -7.43 | 184. | -3.0 | -16.9 | 60.3 | 61.4 |
| Jezero Crater: ESP_088562_1985 ESP_089208_1985 (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 | 18.47 | 77.4 | -8.9 | 15.11 | 48.1 | 47.9 |
| Gullies on Western Wall of Nier Crater: ESP_088574_2230 ESP_088640_2230 (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 | 42.77 | 105. | -0.5 | -17.0 | 44.0 | 45.8 |
Page 35 of 896 (8,955 images) | |||||