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
Eberswalde Crater: PSP_001600_1560 PSP_002233_1560 (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
-23.7	326.	-24.	3.455	67.5	61.6
Uzboi Vallis Breach in Holden Crater Rim: PSP_003288_1530 PSP_003710_1530 (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
-26.9	325.	0	-11.1	52.9	48.7
Light-toned Layering along Plains and in Pit floor Next to Juventae Chasma: PSP_004990_1755 ESP_012255_1755 (Interval in Earth days: 566)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.64	296.	-3.4	23.55	39.1	53.5
Interior of Western Candor Chasma: PSP_003474_1735 PSP_003540_1735 (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
-6.44	283.	17.0	-6.73	51.8	53.2
Proposed MSL Site in Southwest Arabia Terra: PSP_002812_1855 ESP_011844_1855 (Interval in Earth days: 704)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.603	355.	5.55	24.45	55.9	56.7
Putative Polyhydrated Sulfate Deposits in East Melas Chasma: PSP_003487_1670 ESP_040936_1670 (Interval in Earth days: 2918)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.6	290.	0	-25.0	51.7	35.6
Faulting within the Layered Deposits in Candor Chasma: PSP_001641_1735 PSP_002063_1735 (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
-6.67	284.	-1.8	23.61	57.4	54.8
Crater in Western Arabia Terra with Stair-Stepped Hills and Dark Dunes: PSP_001902_1890 PSP_002047_1890 (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
8.814	-1.0	11.6	25.47	52.0	51.3
Depositional Fan : PSP_002387_1985 PSP_003798_1985 (Interval in Earth days: 110)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.48	77.4	1.71	-15.8	55.6	63.7
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