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

Strike Slip Fault in Amazonis Planitia: PSP_009463_2010 PSP_009608_2010 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
20.81	200.	-2.4	11.28	47.0	46.3
Dry Cataracts in Athabasca Valles: PSP_009702_1900 PSP_009847_1900 (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
9.873	156.	0.40	15.92	51.2	50.3
Well-Preserved Crater on a Steep Slope in Tyrrhena Terra: PSP_009824_1610 PSP_010246_1610 (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
-18.5	69.0	6.12	-5.57	65.8	65.3
Layering in Gigas Sulci: PSP_009330_1875 ESP_062208_1875 (Interval in Earth days: 4120)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.582	232.	4.36	-6.52	51.2	50.1
Exposure of Light-Toned Layering along Wallrock in Coprates Chasma: PSP_009684_1695 PSP_010396_1695 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.2	290.	-2.2	19.86	61.5	58.8
Pit and Channel on Southwestern Pavonis Mons: PSP_009923_1785 PSP_010213_1785 (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
-1.67	246.	-21.	14.06	58.1	55.7
Central Pit of Large But Well-Preserved Crater: PSP_009585_1660 PSP_010429_1660 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.7	113.	5.01	-19.0	63.2	63.2
Distributaries From Athabasca Valles: PSP_009768_1880 PSP_010045_1880 (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
7.721	154.	7.98	-19.7	51.6	54.3
Small Crater on the North Polar Deposits: PSP_009773_2675 PSP_010500_2675 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.25	297.	0.08	-14.1	65.4	73.7
High-Latitude Exposure of North Polar Layered Deposits: PSP_009309_2725 PSP_009589_2675 (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
87.52	327.	-4.7	-14.4	64.2	64.4
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