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

Fresh Impact Crater in Utopia Planitia: ESP_011287_2165 ESP_011564_2165 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.02	80.5	-2.6	-23.3	62.3	67.7
Crater in Meridiani Planum with Layering: ESP_011277_1825 ESP_011910_1825 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.221	357.	3.65	-14.2	56.8	59.2
Fan at Valley Mouth: PSP_010434_1575 ESP_045431_1575 (Interval in Earth days: 2727)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-22.3	336.	2.50	-20.1	66.0	64.0
Terraced Fan in Aeolis Region: PSP_009729_1735 ESP_015953_1735 (Interval in Earth days: 485)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.53	141.	5.81	-16.3	58.8	45.4
Aprons with Channels in Eos Chasma: PSP_009327_1665 PSP_009960_1665 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.3	317.	0	-20.9	63.3	64.2
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
Cones at Edge of North Polar Layered Deposits: PSP_009630_2590 PSP_009670_2590 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
79.00	299.	8.09	-15.1	58.0	59.9
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
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
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