HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

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.

Stereo Pair List (csv) Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Mass Wasting Feature on Southern Wall of Crater Near Amazonis Mensa : ESP_059611_1860 ESP_060244_1860 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.755	207.	5.84	-4.61	33.9	39.7
A Snow Plow Landslide : ESP_058960_1800 ESP_058894_1800 (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
-0.05	341.	-2.6	20.52	31.7	29.8
Channels and Lobe Deposits : ESP_059421_2170 ESP_060265_2170 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.74	350.	6.00	-5.80	45.1	40.8
Well-Preserved Small Impact Crater on Hellas Planitia Floor : ESP_059261_1380 ESP_067886_1380 (Interval in Earth days: 672)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.7	49.7	-4.4	21.24	51.7	52.2
Fractured Ground in Aram Chaos : ESP_059237_1830 ESP_059382_1830 (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
2.925	339.	-8.7	7.4	33.2	32.5
Large Channel East of Majuro Crater : ESP_059497_1465 ESP_059431_1465 (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
-32.9	85.0	-0.7	18.93	49.3	47.1
Possible Sulfate-Rich Terrain : ESP_059463_1730 ESP_059041_1730 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.94	290.	-7.8	7.619	35.8	31.0
Terminus of Pitted Materials Emanating from Oudemans Crater : ESP_059411_1735 ESP_059266_1735 (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
-6.34	269.	2.11	-14.5	34.4	34.3
Floor of Nicholson Crater : ESP_059295_1795 ESP_059361_1795 (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
-0.27	195.	2.88	-19.5	32.4	34.7
Impact Crater with Central Pit : ESP_059263_1840 ESP_059408_1840 (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
4.060	349.	-8.6	7.628	33.4	32.6
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