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
Slope Streaks in Terra Sabaea South of Janssen Crater: PSP_003694_1800 ESP_030409_1800 (Interval in Earth days: 2081)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.082	37.9	-4.8	-27.3	54.3	53.4
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
Small Scallops Suggesting Sublimation O North Bank of Auqakuh Vallis: PSP_003482_2115 PSP_005895_2115 (Interval in Earth days: 188)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
31.05	60.7	6.34	26.06	68.8	48.6
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
Cerberus Fossae and Diverse Morphologies: PSP_003241_1880 PSP_003531_1880 (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
7.700	164.	-6.5	25.78	58.2	55.6
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
Exposure of South Polar Layered Deposit: PSP_003341_0935 PSP_003406_0935 (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
-86.4	9.61	-0.0	16.50	75.3	72.7
Comparative Gully Morphology: PSP_003557_1335 PSP_004058_1335 (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
-46.1	183.	1.07	19.97	52.5	43.7
	Page 861 of 891 (8,901 images)