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

Split Slope Streak in Unnamed Arabia Terra Crater: PSP_008507_1825 PSP_008942_1825 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.346	26.9	-7.7	3.77	52.3	53.1
Coprates Chasma Debris Flow Aprons: PSP_008906_1685 PSP_009763_1685 (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
-11.3	292.	-6.3	18.11	61.8	60.7
Potential Phyllosilicates in Acidalia Region: PSP_009182_2215 PSP_009472_2215 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.28	309.	-4.4	16.00	43.6	43.0
Stratigraphy Exposed in Crater Wall: PSP_009048_1965 PSP_010037_1965 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.47	11.6	-4.7	-17.5	47.5	51.5
Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_008680_2050 PSP_009260_2050 (Interval in Earth days: 46)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.63	340.	-11.	19.88	44.5	43.4
Textured Plain in Arcadia Planitia: PSP_008566_2285 ESP_016069_2285 (Interval in Earth days: 585)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
48.18	209.	-4.0	-26.0	43.4	49.7
Central Peak of Bonestell Crater: PSP_008733_2225 ESP_018372_2225 (Interval in Earth days: 752)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.96	329.	-2.7	11.77	42.5	43.0
Dune Interaction with Topography in Ganges Chasma: PSP_008536_1725 PSP_009604_1725 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.40	314.	8.72	-5.05	56.9	60.1
Merging Lobate Debris Aprons of Deuteronilus Mensae: PSP_008744_2240 PSP_009535_2240 (Interval in Earth days: 62)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.76	29.3	-6.2	15.83	43.0	43.5
Polar Layered Deposits Unconformity: PSP_009203_2625 PSP_009585_2625 (Interval in Earth days: 30)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
82.34	79.7	-7.1	7.321	58.9	59.8
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