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

Flow Feature on Eos Chasma Wall: PSP_007389_1665 ESP_026324_1665 (Interval in Earth days: 1475)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.4	317.	-2.5	19.41	51.1	59.2
Possible Sulfates in Ius Chasma: PSP_007509_1720 ESP_050839_1720 (Interval in Earth days: 3376)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.70	279.	-2.3	13.43	49.3	36.5
Interesting Periglacial Assemblage in Utopia Planitia: PSP_007384_2225 PSP_009467_2225 (Interval in Earth days: 163)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
42.22	86.3	-1.0	14.43	44.2	43.1
Santa Fe Crater in Chryse Planitia: PSP_007244_1995 ESP_016052_1995 (Interval in Earth days: 687)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.19	311.	5.51	19.74	38.9	37.5
Fresh Rayed Crater: PSP_007707_1600 ESP_071927_1600 (Interval in Earth days: 5003)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.5	274.	-2.6	15.67	58.5	65.0
Center of Mars: PSP_007361_1800 ESP_041909_1800 (Interval in Earth days: 2692)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.01	0.00	-0.1	20.55	44.1	35.7
Fresh Double-Layered Ejecta Crater: PSP_007947_2350 PSP_009160_2350 (Interval in Earth days: 95)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
54.48	190.	0.23	-18.0	46.6	47.1
Well-Exposed Scarp of Noachian Phyllosilicates Along Nili Fossae: PSP_007200_2005 ESP_016153_2005 (Interval in Earth days: 698)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
20.03	73.6	1.53	26.79	39.1	37.1
Wall Layers of Tooting Crater: PSP_007907_2035 ESP_019115_2035 (Interval in Earth days: 873)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.18	208.	-2.3	5.434	41.6	48.0
Fresh 10-Kilometer Diameter Unnamed Crater in Terra Sabaea: PSP_007966_1615 ESP_025055_1615 (Interval in Earth days: 1331)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.1	41.5	5.02	25.73	59.9	51.0
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