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

Dune Migration: ESP_027738_2590 ESP_027646_2590 (Interval in Earth days: 7)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
78.99	212.	7.64	-8.70	62.0	62.1
Northern Residual Cap Crater: ESP_027635_2680 ESP_028042_2680 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.94	134.	-17.	-7.27	68.2	73.0
Dune Migration: ESP_027412_2600 ESP_027320_2600 (Interval in Earth days: 7)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
79.98	110.	6.47	-8.84	59.6	59.8
Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor: ESP_027771_1640 ESP_028470_1640 (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
-15.7	56.6	8.78	-7.44	61.0	59.4
Layered Flow Ejecta: ESP_027668_1805 ESP_028446_1795 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.26	349.	-24.	1.845	55.6	53.7
Small Crater on the North Polar Deposits: ESP_027748_2675 ESP_036120_2675 (Interval in Earth days: 653)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.25	297.	-17.	-5.14	68.9	64.4
Tilted Block on Olympus Mons Scarp: ESP_027712_2035 ESP_028279_2035 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.21	223.	-6.3	15.88	47.0	49.0
Possible Future Landing Site in Sabrina Vallis Outlet: ESP_027656_1920 ESP_027168_1920 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.87	313.	-3.6	13.23	49.2	46.9
Overlapping Pedestal Craters in THEMIS Image V29326005: ESP_027413_2355 ESP_027967_2355 (Interval in Earth days: 43)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
55.13	98.5	7.76	-8.98	47.1	54.2
North Polar Gypsum Dune Changes: ESP_027474_2610 ESP_027935_2610 (Interval in Earth days: 36)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
80.83	223.	-6.5	17.65	61.4	65.0
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