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

Surface Morphology on Floor of Antoniadi Crater : ESP_043555_2035 ESP_043700_2035 (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
23.20	60.0	-4.4	11.69	40.8	39.6
Flows on Fracture in Adamas Labyrinthus : ESP_043672_2170 ESP_044371_2170 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.77	103.	-0.0	-18.1	39.5	41.4
Western Interior of Tooting Crater : ESP_043721_2035 ESP_043866_2035 (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
23.18	207.	2.34	18.38	40.5	39.3
USGS Dune Database Entry Number 0795-196 Changes : ESP_043607_2000 ESP_044385_2000 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.67	79.5	9.89	22.91	40.5	40.5
Columbia Hills Candidate Landing Site for 2020 Mission : ESP_043551_1655 ESP_043696_1655 (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
-14.4	175.	-24.	-7.34	60.0	59.6
Northern Plains Crater Modification : ESP_043549_2265 ESP_043615_2265 (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
45.99	220.	-5.7	-18.9	41.7	42.7
Sharp Albedo Variations on Lobate Debris Apron in Tempe Region : ESP_043534_2230 ESP_043613_2230 (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
42.83	271.	-8.2	18.47	41.1	38.7
Mars 2020 Candidate Landing Site in Nili Fossae : ESP_043528_2020 ESP_043673_2020 (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
21.87	78.5	-17.	-1.93	42.1	41.0
Pit Near Elysium Mons : ESP_043763_2100 ESP_071022_2100 (Interval in Earth days: 2124)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
29.69	139.	10.5	-3.75	38.7	47.6
Nili Patera : ESP_043779_1890 ESP_043423_1890 (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
8.700	67.3	-13.	-25.7	46.9	46.7
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