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

Crater and Ice-Rich Terrain: ESP_086346_2250 ESP_086992_2250 (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
44.64	95.4	-5.9	13.11	49.1	43.8
Features around Cerberus Palus: ESP_086252_1850 ESP_086819_1850 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.904	146.	5.75	-7.57	39.5	45.0
Light-Toned Exposures in Capri Chasma: ESP_086246_1670 ESP_086312_1670 (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
-13.0	312.	9.05	-17.0	45.0	47.7
North-Pole-Facing Deposit in Crater: ESP_086208_2275 ESP_086841_2275 (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
47.24	261.	5.23	-18.4	51.0	48.1
Impact Monitoring in Arcadia Planitia: ESP_086330_2205 ESP_089389_2205 (Interval in Earth days: 238)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.34	173.	-8.4	7.166	47.3	47.9
Lethe Vallis Chevron Shaped Landforms: ESP_086344_1840 ESP_086845_1840 (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
4.028	155.	-7.9	5.786	41.4	44.5
Trough in Nilosyrtis Mensae: ESP_086255_2300 ESP_086888_2300 (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
49.43	59.1	-3.7	-23.5	52.4	49.3
Head of Lethe Vallis: ESP_086199_1840 ESP_087056_1840 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.785	153.	5.44	20.19	39.3	45.1
Deuteronilus Mensae: ESP_086256_2255 ESP_085676_2255 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
45.16	28.6	25.3	-1.94	47.9	56.0
Young Impact on Layers in Protonilus Mensae: ESP_086295_2230 ESP_086717_2230 (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
42.61	46.9	5.28	-12.4	47.7	46.4
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