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.
| Nicholson Crater: ESP_064530_1800 ESP_064807_1800 (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 | 0.058 | 195. | -0.4 | -23.4 | 57.6 | 59.8 |
| Gully Monitoring: ESP_064726_1390 ESP_065491_1390 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.8 | 249. | -0.4 | -21.8 | 61.0 | 52.1 |
| Valleys in Crater Northeast of Argyre Planitia: ESP_064736_1500 ESP_064591_1500 (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 | -29.7 | 335. | 0.30 | -16.8 | 58.2 | 61.0 |
| Channels with Tributaries on Rocky Plains Northwest of Argyre Region: ESP_064645_1320 ESP_082568_1320 (Interval in Earth days: 1397) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.5 | 301. | 5.97 | -6.62 | 63.9 | 60.6 |
| Sublimation at Spiders Site: ESP_064785_0930 ESP_064639_0930 (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 | -87.0 | 127. | 8.53 | 21.89 | 80.1 | 81.5 |
| Fractures and Inlet Valley : ESP_064798_1990 ESP_064653_1990 (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 | 18.64 | 76.2 | 0.85 | -16.8 | 62.7 | 63.1 |
| Network of Sinuous Ridges in Aeolis Dorsa: ESP_064848_1730 ESP_073039_1730 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.70 | 154. | 4.51 | -24.5 | 56.4 | 60.0 |
| Sinuous Ridge Feature in CTX D21_035468_1545_XN_25S202W: ESP_064716_1535 ESP_047534_1535 (Interval in Earth days: 1339) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.2 | 158. | 26.4 | 2.235 | 55.6 | 47.5 |
| Small Barchan Dunes in Northeast Argyre Region: ESP_064789_1350 ESP_064723_1350 (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 | -44.6 | 331. | -5.9 | 10.38 | 61.7 | 61.4 |
| Smooth Area in Phlegra Montes: ESP_064531_2155 ESP_064465_2155 (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 | 35.29 | 164. | -8.4 | 8.287 | 67.0 | 64.8 |
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