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

Light-Toned Layers in Noctis Labyrithus: PSP_006890_1695 ESP_015975_1695 (Interval in Earth days: 708)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.4	261.	2.52	-22.8	42.9	48.0
Survey South Polar Layered Deposits: PSP_004593_0830 PSP_004984_0970 (Interval in Earth days: 30)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-82.6	140.	0	-19.2	72.1	65.8
Possible Exposure of Polar Layered Deposits in Area Not Well Observed: PSP_004882_0880 PSP_004894_0920 (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
-88.1	121.	11.7	11.47	68.6	67.9
Seasonal Monitoring: PSP_005553_0980 PSP_005790_0980 (Interval in Earth days: 18)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-82.1	75.6	-8.4	8.644	71.5	74.2
Large Region of Layering in Meridiani Planum: PSP_006227_1810 ESP_011791_1810 (Interval in Earth days: 434)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
1.126	2.68	0	28.55	34.9	55.4
Layers at the Head of Chasma Australe Exposed over 270 Degrees of Azimuth: PSP_004788_0945 PSP_005079_0945 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-85.6	95.5	0	-16.3	65.3	69.7
Flat-Topped Mound in Utopia Region: PSP_006882_2245 ESP_050990_2240 (Interval in Earth days: 3437)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.97	112.	7.17	-5.64	47.8	46.8
Unnamed Well-Preserved Crater in Cimmeria Terra: PSP_005286_1480 PSP_005576_1480 (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
-31.5	140.	-27.	-1.66	36.8	36.4
Exposure of High-Latitude Polar Layered Deposits Not Well-Observed: PSP_005139_0920 PSP_005269_0920 (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
-87.7	280.	5.03	18.59	70.9	70.7
North Mamers Vallis Proposed Shoreline: PSP_005989_2270 PSP_006912_2270 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
46.44	14.1	5.27	-4.81	60.0	49.8
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