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

Mangala Valles Cataract: PSP_003991_1645 PSP_004347_1645 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.3	210.	0	10.73	46.2	41.2
Unnamed Well-Preserved Crater within the Isidis Basin: PSP_003560_1900 PSP_005828_1900 (Interval in Earth days: 177)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.16	94.5	0.61	10.89	58.6	37.6
Relatively Large Primary Crater on Elysiu Planitia Young Lavas: PSP_003267_1870 PSP_003412_1870 (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
7.153	174.	-3.8	14.59	57.8	56.4
Light-Toned Outcrops in the Plains Between Melas and Candor Chasma: PSP_004318_1730 PSP_004740_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
-6.84	282.	-3.1	-15.3	45.8	41.7
Subset of Gullies Previously Identified in Dunes in MOC Image M19-01170: PSP_003682_1250 PSP_003748_1250 (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
-54.5	12.8	0.14	-13.7	53.3	53.3
Light-Toned Layering in Plains West of Juventae Chasma: PSP_003434_1755 PSP_003579_1755 (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
-4.65	296.	1.00	16.62	53.6	51.7
Odd Layered and Eroding Crater Fill in Deeply Eroded Craters: PSP_003773_1630 PSP_003918_1630 (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
-16.8	42.7	1.82	18.06	48.1	45.3
Light-Toned Layering in Labyrinthus Noctis Pit: PSP_003910_1685 PSP_005400_1685 (Interval in Earth days: 116)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.1	261.	0	14.87	48.2	32.3
Northwest Candor Mensa: PSP_004186_1740 PSP_005597_1740 (Interval in Earth days: 110)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.11	286.	0.29	-24.8	47.3	35.8
Sample Gigas Fossae: PSP_003410_1840 PSP_003832_1840 (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
3.778	230.	7.27	-6.05	55.8	55.2
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