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

Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (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
24.05	63.0	-0.2	13.32	44.2	43.5
Repeated Sulfate and Clay Beds in West Gale Crater: ESP_017786_1745 ESP_017931_1745 (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
-5.36	137.	-13.	1.249	57.9	57.2
Source for Enigmatic Channel in Ceraunius Fossae: ESP_017874_2025 ESP_018296_2025 (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
22.16	248.	13.5	-0.70	43.1	45.2
Layered Deposits in Crater in Western Arabia Terra: ESP_017936_1890 ESP_060489_1890 (Interval in Earth days: 3315)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.810	-0.9	0.22	-9.82	49.5	41.2
Toro Crater Floor Deposits: ESP_017841_1970 ESP_018474_1970 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.31	71.7	-1.4	-21.7	45.8	48.8
Possible MSL Rover Landing Site in South Eberswalde Crater: ESP_018056_1555 ESP_018557_1555 (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
-24.2	326.	3.37	25.76	69.6	67.3
Rocky Flow Lobe From Impact Crater in Tyrrhena Terra: ESP_017998_1765 ESP_053667_1760 (Interval in Earth days: 2780)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-3.64	107.	5.38	27.65	56.0	52.2
Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_017822_2375 ESP_018046_2375 (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
57.37	225.	-10.	14.65	46.4	44.8
Cones at Edge of North Polar Layered Deposits: ESP_017833_2615 ESP_018070_2615 (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
81.25	272.	-6.5	8.031	57.9	57.5
Layered Terrain in Aeolis and Zephyria Regions: ESP_017825_1760 ESP_018458_1760 (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
-3.75	149.	13.9	-9.22	55.2	57.1
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