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

Raised Polygonal Ridges and Light-Toned Material in Syrtis Region: ESP_018065_1975 ESP_019133_1975 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.49	76.4	-5.2	15.52	46.5	48.0
Fresh Looking Crater West of Erebus Montes in Arcadia Planitia: ESP_017784_2185 ESP_018272_2185 (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
38.05	184.	7.20	-20.5	41.1	45.1
Rampart Crater Sample: ESP_018010_2455 ESP_018656_2455 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
65.42	128.	2.96	17.4	49.0	51.6
Exposure of Polar Layered Deposits: ESP_018043_2715 ESP_018084_2685 (Interval in Earth days: 3)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
88.51	196.	-13.	-12.9	64.5	63.9
Central Peak of a Large Crater in Acidalia Planitia: ESP_017700_2160 ESP_018412_2160 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
35.81	319.	-4.0	7.082	42.0	43.2
Valleys and Layering along Melas Region: ESP_018018_1705 ESP_026866_1705 (Interval in Earth days: 689)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.55	283.	-6.8	-17.8	60.4	60.2
Northern Hemisphere Gully Alcoves Seen in MOC Image R16-01542: ESP_017778_2200 ESP_018279_2200 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.87	349.	-7.4	8.255	42.5	42.6
Well-Preserved Impact Crater with Ridges: ESP_017975_1705 ESP_025557_1705 (Interval in Earth days: 590)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.51	16.4	0.77	18.29	59.9	51.6
Exposures of Various North Polar Geologic Units: ESP_017845_2625 ESP_018016_2625 (Interval in Earth days: 13)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
82.42	302.	-5.5	9.318	58.6	58.2
Shallow Channel Cutting through a Crater in CTX Image: ESP_017740_2230 ESP_024900_2230 (Interval in Earth days: 558)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
42.79	305.	3.34	18.77	41.7	42.4
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