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.
| Crescentic Feature on South Polar Layered Deposits : ESP_057951_0925 ESP_057831_0925 (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 | -87.6 | 240. | 7.09 | 20.50 | 68.9 | 66.4 |
| Impact Crater : ESP_058133_1175 ESP_058212_1175 (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 | -62.2 | 252. | -4.1 | 13.22 | 50.1 | 50.1 |
| Western Rim of Rayed Crater in Daedalia Planum : ESP_058094_1565 ESP_067721_1565 (Interval in Earth days: 750) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 230. | 0.94 | 10.31 | 30.2 | 41.6 |
| Exposure of South Polar Layered Deposits : ESP_058100_0915 ESP_057624_0915 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.4 | 122. | 19.8 | 27.08 | 70.4 | 65.0 |
| South Polar Layered Deposits : ESP_057953_0925 ESP_058440_0925 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.5 | 179. | 7.63 | 16.48 | 68.7 | 74.3 |
| Possible Exposures of Polar Layered Deposits in Area Not Well Observed : ESP_058154_0920 ESP_057968_0920 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 84.6 | 17.3 | 29.61 | 70.9 | 67.6 |
| Pitted Cones in Chryse Planitia : ESP_057932_2140 ESP_058077_2140 (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 | 33.80 | 325. | -2.1 | 16.70 | 62.5 | 59.7 |
| Pitted Dunes : ESP_058019_1245 ESP_065878_1245 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.3 | 123. | -6.2 | 27.59 | 44.2 | 46.9 |
| South Polar Layered Deposits : ESP_057957_0925 ESP_058143_0875 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 101. | 3.59 | 9.556 | 70.0 | 73.2 |
| Channel East of Majuro Crater : ESP_058073_1465 ESP_058864_1465 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.3 | 84.9 | 0.97 | 21.34 | 32.3 | 38.1 |
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