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.
Large Polygons in Deuteronilus Mensae: PSP_007492_2265 PSP_007703_2265 (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 | 46.12 | 15.5 | 7.95 | -4.50 | 44.6 | 44.7 |
Relict Glacial Landform in Deuteronilus Mensae: PSP_006806_2215 PSP_007096_2215 (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 | 41.15 | 29.5 | -8.5 | 7.997 | 47.9 | 44.7 |
Landslide in Xanthe Terra: PSP_005701_1920 ESP_050033_1920 (Interval in Earth days: 3455) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.72 | 322. | -4.5 | 26.31 | 40.5 | 34.0 |
Layered Bedrock with Possible Hydrated Sulfates: PSP_007403_1670 PSP_008194_1670 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.9 | 295. | -5.3 | 5.733 | 51.1 | 58.4 |
Inverted Fluvial Channels and Craters with Ejecta Rays: PSP_007394_1750 ESP_019736_1750 (Interval in Earth days: 962) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.23 | 180. | -8.0 | -23.2 | 47.2 | 57.6 |
Chasm in Gale Crater's Interior Mound: PSP_006855_1750 PSP_007501_1750 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.09 | 137. | -6.5 | 5.424 | 41.0 | 47.3 |
Proposed MSL Landing Site in Miyamoto Crater: PSP_006913_1765 PSP_010196_1765 (Interval in Earth days: 255) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.27 | 352. | 7.82 | -6.94 | 40.0 | 57.9 |
Proposed MSL Landing Site in Mawrth Vallis - Ellipse 4: PSP_006887_2050 PSP_007823_2050 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.85 | 339. | -2.9 | 18.09 | 40.1 | 39.4 |
Proposed MSL Landing Site in Mawrth Vallis Region: PSP_006676_2045 PSP_007612_2045 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.03 | 341. | -7.4 | 19.15 | 40.7 | 38.8 |
Streamlined Features: PSP_006677_1475 PSP_006967_1475 (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 | -32.4 | 320. | -3.6 | 17.23 | 52.2 | 55.7 |
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