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

Exposure of Polar Layered Deposits Not Well Covered by Mars Global Surveyor: PSP_001342_2680 PSP_001568_2680 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
88.04	62.4	-6.0	-13.1	70.2	72.6
Boulder Tracks with Boulders at Ends: PSP_001730_1740 PSP_002086_1740 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.87	16.4	-2.4	21.5	57.0	54.7
Fresh-Looking Gullies: PSP_001714_2390 PSP_001846_2390 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
58.73	82.3	3.50	-8.24	57.8	60.7
Possible Phoenix Lander Landing Site: TRA_000881_2475 TRA_000894_2475 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
67.49	130.	-21.	0	54.8	53.1
Interior Channel in Parana Valles: PSP_002008_1560 PSP_002285_1560 (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
-23.9	350.	-0.6	-27.3	63.5	63.7
White Rock Deposits: PSP_002033_1720 PSP_002099_1720 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.01	25.0	5.96	-17.5	56.7	58.4
Knobs Near Arrhenius Region : PSP_002478_1365 PSP_003678_1365 (Interval in Earth days: 94)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.9	120.	4.1	-7.1	67.2	50.4
Northern Plains Sample: PSP_001959_2485 PSP_002091_2485 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
68.15	232.	0.57	-14.1	66.1	69.5
Tooting Crater West Rim and Ejecta : PSP_002580_2035 PSP_002646_2035 (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
23.15	207.	3.51	-16.7	58.0	60.3
Gamboa Crater Central Uplift in Acidalia Planitia : PSP_002721_2210 ESP_028724_2210 (Interval in Earth days: 2026)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.77	315.	0.64	-12.1	66.1	59.9
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