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 Outcrops in the Plains Between Melas and Candor Chasma: PSP_004318_1730 PSP_004740_1730 (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
-6.84	282.	-3.1	-15.3	45.8	41.7
Mangala Valles Cataract: PSP_003991_1645 PSP_004347_1645 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.3	210.	0	10.73	46.2	41.2
Unnamed Well-Preserved Crater within the Isidis Basin: PSP_003560_1900 PSP_005828_1900 (Interval in Earth days: 177)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.16	94.5	0.61	10.89	58.6	37.6
Light-Toned Layering in Labyrinthus Noctis Pit: PSP_003910_1685 PSP_005400_1685 (Interval in Earth days: 116)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.1	261.	0	14.87	48.2	32.3
Dark Rimless Pits in Tharsis: PSP_003317_1975 ESP_019997_1975 (Interval in Earth days: 1300)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.26	247.	3.53	26.79	61.3	52.5
Fresh Crater: PSP_003942_1585 ESP_058138_1585 (Interval in Earth days: 4223)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.1	109.	1.8	-11.9	45.4	31.0
Subset of Gullies Previously Identified in Dunes in MOC Image M19-01170: PSP_003682_1250 PSP_003748_1250 (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
-54.5	12.8	0.14	-13.7	53.3	53.3
Layers Exposed in the Central Uplift of an Unnamed Crater: PSP_003803_1515 ESP_013679_1515 (Interval in Earth days: 770)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.3	304.	5.29	-11.0	46.2	36.5
Slope Streaks in Terra Sabaea South of Janssen Crater: PSP_003694_1800 ESP_030409_1800 (Interval in Earth days: 2081)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.082	37.9	-4.8	-27.3	54.3	53.4
Western Region of Zunil Crater: PSP_004309_1880 ESP_020211_1880 (Interval in Earth days: 1239)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.728	166.	4.71	29.29	53.0	52.5
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