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

Fans in 10-Kilometer Diameter Crater North of Mojave Crater: ESP_026983_1910 ESP_027682_1910 (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
10.77	325.	-1.3	-18.7	48.1	50.8
Candidate Future Landing Site Near Sabrina Vallis: ESP_026812_1920 ESP_026878_1920 (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
11.75	313.	-1.3	-21.3	47.4	49.1
Layers in Danielson Crater: ESP_026626_1885 ESP_026349_1885 (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
8.278	352.	-18.	8.638	49.9	47.0
Terrain Near Mareotis Fossae: ESP_026918_2310 ESP_027472_2310 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
50.71	293.	0	-23.3	43.5	48.9
Rayed Crater: ESP_026937_2145 ESP_027847_2145 (Interval in Earth days: 71)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.12	137.	-0.8	-12.9	41.9	48.3
Dunes and North Polar Outlier: ESP_026634_2595 ESP_026528_2595 (Interval in Earth days: 8)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
79.16	125.	-21.	5.115	57.5	55.7
South Coprates Chasma Dune Changes: ESP_026905_1660 ESP_027182_1660 (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
-14.0	296.	6.57	-16.4	61.6	62.9
Cones at Edge of North Polar Layered Deposits: ESP_026931_2600 ESP_027234_2600 (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
79.99	289.	-8.6	6.229	57.7	58.3
Northern Plains Craters: ESP_026987_2305 ESP_027264_2305 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
50.36	208.	11.3	-1.28	42.7	45.3
Sinuous Ridges with Different Morphologies in Aeolis Planum: ESP_026818_1740 ESP_026462_1740 (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
-6.09	150.	6.46	-7.25	56.4	56.5
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