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.
| Hadriacus Mons Southwestern Caldera Wall: ESP_077446_1490 ESP_085674_1490 (Interval in Earth days: 642) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.6 | 92.4 | -8.3 | 6.14 | 56.7 | 46.3 |
| Ejecta of Well-Preserved 12-Kilometer Impact Crater in South Utopia Planitia: ESP_077194_2070 ESP_077260_2070 (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 | 26.82 | 120. | 4.00 | -7.09 | 42.5 | 43.1 |
| Small Delta or Fan: ESP_076752_2155 ESP_076198_2155 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.94 | 302. | -2.9 | 8.438 | 50.6 | 56.7 |
| Valley South of Ares Vallis: ESP_076896_1890 ESP_076962_1890 (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 | 9.103 | 335. | 8.83 | -5.66 | 37.4 | 38.6 |
| Lower Interior Layered Deposits in Eastern Candor Chasma: ESP_076845_1730 ESP_076911_1730 (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 | -6.94 | 288. | 8.48 | -6.96 | 36.9 | 38.6 |
| Terrain Sample in Claritas Fossae: ESP_076767_1510 ESP_076833_1510 (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 | -28.5 | 260. | 10.3 | -4.76 | 43.7 | 45.6 |
| Jezero Crater Inlet Valley: ESP_077011_1990 ESP_077077_1990 (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 | 18.63 | 76.3 | -2.1 | -15.0 | 40.6 | 41.5 |
| Layered Deposits in Impact Crater in Utopia Planitia: ESP_076984_2240 ESP_077960_2240 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.81 | 89.5 | -1.1 | -11.8 | 53.7 | 46.9 |
| Ripple Change Detection of Gullied Dunes in Southern Mid-Latitudes: ESP_076842_1275 ESP_076710_1275 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -51.9 | 18.1 | -1.8 | 18.56 | 60.6 | 57.2 |
| Channels in Rahway Valles: ESP_076981_1890 ESP_076770_1890 (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 | 8.810 | 175. | 11.0 | -7.15 | 37.2 | 38.5 |
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