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

Rayed Crater on Southeast Flank of Elysium Mons: PSP_009333_2025 PSP_009834_2025 (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
22.46	151.	-21.	-0.87	47.7	47.8
Scarp-Fed Dark Dunes: PSP_009885_2655 PSP_010344_2655 (Interval in Earth days: 36)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
85.68	179.	-14.	15.88	65.5	70.3
Flow on Floor of Kasei Valles: PSP_010000_2055 ESP_069104_2055 (Interval in Earth days: 4605)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.17	299.	0	22.72	48.1	44.8
Murgoo Crater: PSP_009801_1565 ESP_053817_1560 (Interval in Earth days: 3429)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.6	337.	5.39	-7.80	69.0	67.0
Light-Toned Layering in Plains South of Melas Chasma: PSP_009948_1700 ESP_015961_1700 (Interval in Earth days: 469)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.89	282.	5.17	-11.2	60.5	46.6
Slope Streaks on Nicholson Crater Mound: PSP_009371_1800 PSP_009516_1800 (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
-0.00	195.	-5.9	9.471	55.9	55.0
Sample Artynia Catena: PSP_009646_2265 ESP_016305_2265 (Interval in Earth days: 519)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
46.32	240.	0	16.73	45.9	43.9
Landslide Alcove Within the Arsia Mons Southwest Rift Zone: PSP_009910_1690 PSP_010543_1690 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.7	239.	17.3	-3.84	60.3	60.4
Layering in Gigas Sulci: PSP_009330_1875 ESP_062208_1875 (Interval in Earth days: 4120)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.582	232.	4.36	-6.52	51.2	50.1
High-Latitude Exposure of North Polar Layered Deposits: PSP_009353_2725 PSP_009553_2675 (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
87.66	228.	-3.3	-16.1	63.7	64.3
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