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.
| Well-Preserved 7-Kilometer Impact Crater : ESP_046334_2075 ESP_050883_2075 (Interval in Earth days: 355) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.00 | 154. | -7.3 | 5.524 | 52.7 | 37.9 |
| Fracture in Utopia Planitia: ESP_046296_2130 ESP_046006_2130 (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 | 32.86 | 109. | 7.91 | -14.7 | 52.5 | 50.8 |
| Alluvial Fans in Southwestern Mojave Crater: ESP_046275_1870 ESP_051958_1870 (Interval in Earth days: 443) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.160 | 326. | 5.60 | 25.31 | 49.5 | 40.4 |
| Crater in Corinto Crater Secondary Field : ESP_046440_1965 ESP_047152_1965 (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 | 16.29 | 140. | 5.52 | 18.67 | 50.8 | 55.2 |
| Crater with Steep Slopes: ESP_046262_2095 ESP_051866_2095 (Interval in Earth days: 436) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.21 | 320. | -8.3 | -22.4 | 52.5 | 39.9 |
| Landforms at West End of Her Desher Vallis : ESP_046579_1550 ESP_047423_1550 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.5 | 311. | 5.67 | -27.2 | 56.1 | 51.0 |
| Floor of East Candor Chasma : ESP_046395_1730 ESP_046250_1730 (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 | -6.84 | 292. | 3.09 | -12.7 | 52.0 | 53.4 |
| Braided Channel System in Eastern Hellas Region : ESP_046323_1405 ESP_051149_1405 (Interval in Earth days: 377) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.9 | 102. | 6.20 | -8.76 | 65.1 | 61.5 |
| Sharply Stratified Wind Eroded Crater Fill Deposit : ESP_046498_1430 ESP_046854_1430 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.4 | 5.63 | -9.7 | 1.604 | 63.0 | 58.0 |
| Protonilus Mensae Debris Apron : ESP_046430_2260 ESP_046496_2260 (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 | 45.90 | 48.9 | 8.77 | -5.59 | 59.3 | 61.5 |
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