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

Bright, Fine Layers in Juventae Chasma: PSP_003790_1755 PSP_004291_1755 (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
-4.61	296.	4.21	28.89	51.2	44.7
MSL Landing Site in Melas Chasma: PSP_002828_1700 ESP_019508_1700 (Interval in Earth days: 1300)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.82	283.	-28.	-5.16	58.0	58.0
Layers in Becquerel Crater: PSP_001546_2015 PSP_001955_2015 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.44	351.	2.47	-5.93	49.3	52.9
High Thermal-Inertia Terrace Blocks in Holden Crater: PSP_005134_1545 PSP_005978_1545 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.4	327.	0	-26.7	33.4	39.9
Layers Exposed in Crater Near Mawrth Vallis: PSP_004052_2045 ESP_012873_2045 (Interval in Earth days: 687)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.30	340.	0	15.95	65.6	65.6
Proposed MSL Site in Meridiani Crater: PSP_002179_1855 ESP_063535_1855 (Interval in Earth days: 4781)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.421	358.	-3.6	18.24	54.7	52.5
Interior Layered Deposits in Candor Chasma : PSP_002696_1745 PSP_003197_1745 (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
-5.69	284.	0.15	26.47	55.7	52.3
Colorful Rocks in the Central Peaks of Ritchey Crater: PSP_005372_1515 PSP_006005_1515 (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
-28.4	309.	7.53	-14.5	33.5	40.6
Layered Deposits in Ritchey Crater: PSP_003249_1510 PSP_003526_1510 (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
-28.5	309.	6.98	-18.0	53.0	51.6
Large Area of Light-Toned Layering at Mawrth Vallis: PSP_001929_2050 PSP_002351_2050 (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
24.96	340.	0	-11.8	52.3	57.4
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