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

Extra-Crater Sinuous Ridge: ESP_072693_2240 ESP_072772_2240 (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
43.67	232.	-2.8	21.12	60.6	59.7
Mounds in Oxia Colles: ESP_072597_2045 ESP_072452_2045 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.46	336.	-1.7	-11.3	55.4	54.9
Monitor Vaduz Crater: ESP_072635_2185 ESP_072701_2185 (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
38.26	15.7	7.55	-10.5	57.4	59.8
Aurorae Chaos: ESP_072769_1715 ESP_072914_1715 (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
-8.40	324.	-6.1	7.57	59.2	57.8
Terrain Sample: ESP_072782_1785 ESP_072927_1785 (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
-1.52	328.	0.87	14.49	57.2	56.2
Ridges in Huygens Crater: ESP_072713_1645 ESP_073135_1645 (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
-15.4	54.0	-2.4	-21.0	61.1	60.7
Small Delta or Fan: ESP_072780_2165 ESP_073070_2165 (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
36.09	17.5	4.29	23.93	59.1	61.2
Recent Impact near Hebrus Valles: ESP_072763_2025 ESP_080662_2025 (Interval in Earth days: 615)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.25	124.	-3.8	12.03	56.9	49.7
Measure Orientations of Layers in Luba Crater: ESP_072479_1615 ESP_072545_1615 (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
-18.3	323.	1.63	-22.3	62.9	64.4
Deposits in Ganges Chasma: ESP_072664_1715 ESP_072743_1715 (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
-8.58	311.	-6.8	28.24	59.5	56.4
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