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.
| Flow Draped over Crater Rim Visible in CTX Image : ESP_025563_1975 ESP_025207_1975 (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 | 17.48 | 209. | 15.2 | 2.131 | 39.4 | 38.8 |
| Fresh Crater on Northern Plains: ESP_025775_2290 ESP_026065_2290 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.83 | 177. | 8.09 | 25.59 | 41.9 | 39.7 |
| Channel in Tharsis Region: ESP_025417_1965 ESP_024916_1965 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.19 | 235. | 17.6 | -8.13 | 38.8 | 38.5 |
| Banded Features in Hellas Region Visible in CTX Image : ESP_025555_1360 ESP_025621_1360 (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 | -43.9 | 78.0 | -7.5 | -22.6 | 77.3 | 78.9 |
| Bedrock Exposed in the Central Uplift of a Unnamed Crater: ESP_025766_2005 ESP_025700_2005 (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 | 20.18 | 69.3 | -7.5 | 11.70 | 41.5 | 39.7 |
| Mesa-Forming Lobes Visible in CTX Image G07_020876_2133: ESP_025623_2130 ESP_026335_2130 (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 | 32.48 | 9.93 | 8.87 | 25.42 | 38.7 | 38.1 |
| Hebrus Valles: ESP_025777_1990 ESP_027254_1990 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.14 | 127. | 9.74 | -19.1 | 40.7 | 47.4 |
| Terrain with Parallel Lineations Visible in THEMIS Image V29600014: ESP_025738_2195 ESP_026582_2195 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.24 | 110. | 2.71 | -14.2 | 40.0 | 42.0 |
| Small Volcanoes Visible in THEMIS Image V27150023: ESP_025773_2250 ESP_027039_2250 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.61 | 233. | 1.74 | -18.1 | 41.1 | 44.3 |
| Small Mounds in Chryse Planitia: ESP_025427_1995 ESP_025282_1995 (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 | 19.37 | 322. | 6.11 | -10.3 | 39.2 | 40.0 |
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