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

Terrain in Crater in Tempe Terra: ESP_088260_2150 ESP_088827_2150 (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
34.74	40.1	2.83	-11.4	42.9	45.9
Dunes in Crater: ESP_088355_2370 ESP_088368_2370 (Interval in Earth days: 2)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
56.69	322.	0.37	27.25	46.2	43.8
Distinct Crater Wall Layers in Oxia Planum: ESP_088236_1995 ESP_087946_1995 (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
19.08	338.	-1.7	-16.6	46.5	47.0
Dune Field: ESP_088070_2535 ESP_088413_2535 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
73.41	178.	0.65	-15.8	53.4	54.6
North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_088186_2175 ESP_088753_2175 (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
37.39	260.	0.31	-14.6	42.8	45.7
Small Fresh Impact Crater: ESP_088159_1670 ESP_088726_1670 (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
-13.0	283.	6.05	-15.1	62.5	64.7
Meander in Channel Southwest of Mamers Valles: ESP_088327_2165 ESP_088538_2165 (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
35.99	10.3	4.70	-6.95	42.9	44.4
Jezero Crater: ESP_088206_1985 ESP_088285_1985 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.47	77.3	-2.3	27.85	46.7	44.3
Monitor Slope in West Coprates Chasma: ESP_088106_1685 ESP_088673_1685 (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
-11.5	290.	5.12	-16.4	61.5	63.9
Alluvial Fans in Kasei Valles: ESP_088264_2035 ESP_088475_2035 (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
23.06	294.	-13.	-26.2	46.4	48.0
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