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

Edge along Gale Crater Interior Mound: PSP_001488_1750 PSP_001752_1750 (Interval in Earth days: 20)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.83	137.	2.36	-16.1	56.5	57.7
Layers in a Central Mound in Gale Crater: PSP_001422_1750 PSP_001620_1750 (Interval in Earth days: 15)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.98	137.	2.01	-12.5	56.7	57.6
Best Fan Surfaces in West Holden Crater: PSP_001468_1535 PSP_002154_1530 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.5	325.	6.55	-10.2	67.8	64.4
Proposed Strandline: PSP_001820_1985 PSP_003442_1985 (Interval in Earth days: 126)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.25	77.3	1.02	-22.9	51.3	64.1
Flow-like Features in Promethei Terra: PSP_005419_1380 PSP_005696_1380 (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
-41.6	108.	-0.9	-24.6	39.8	44.5
Chain of Pits on Arsia Mons: PSP_005414_1735 ESP_011756_1735 (Interval in Earth days: 494)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.52	240.	3.62	20.67	34.2	55.5
Channels East of Olympus Mons: PSP_005401_1960 PSP_005546_1960 (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
15.99	232.	-5.7	8.395	46.2	43.7
Small Winding Channel in Tartarus Colles: PSP_001420_2045 ESP_069174_2045 (Interval in Earth days: 5279)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.47	188.	7.84	27.97	47.7	44.4
Gullies in Mantle Terrain in Sisyphi Planum: PSP_005160_1150 PSP_005595_1150 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-64.8	344.	0	20.43	52.1	56.4
Cratered Cones Near Hephaestus Fossae: PSP_004060_2020 ESP_057069_2020 (Interval in Earth days: 4131)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.73	121.	9.17	-20.1	63.3	62.5
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