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

Multiple Geomorphic and Geologic Units in Southern Meridiani Planum : ESP_044665_1785 ESP_069445_1785 (Interval in Earth days: 1931)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.58	0.32	8.50	-23.2	51.9	57.4
Atypical Landform among Dunes in Polar Erg : ESP_044917_2575 ESP_044864_2575 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
77.54	307.	-7.0	8.026	57.6	56.4
Candidate Landing Site for 2020 Mission : ESP_044896_1650 ESP_044751_1650 (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
-14.7	175.	16.8	-6.7	59.1	60.9
Terraced Crater in Amazonis Planitia : ESP_044697_2090 ESP_044974_2090 (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
28.64	203.	-2.8	-14.9	41.1	42.9
Exposure of North Polar Layered Deposits : ESP_044783_2585 ESP_053341_2585 (Interval in Earth days: 666)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
78.57	1.01	0.17	-19.9	57.0	57.3
Plains North of Tempe Terra : ESP_044813_2320 ESP_045380_2320 (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
51.67	275.	-12.	8.373	44.7	47.1
Possible Chloride Deposit Disrupted By Simple Crater : ESP_044929_1495 ESP_052880_1495 (Interval in Earth days: 619)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-30.3	358.	0	24.50	70.8	70.3
Wrinkle Ridge and Channel Intersection along Huygens Crater Rim : ESP_044729_1600 ESP_045006_1600 (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
-19.8	56.3	-1.0	-15.5	64.2	64.1
Possible Gray Hematite in Capri Chasma : ESP_044891_1665 ESP_045313_1665 (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
-13.3	313.	1.73	14.11	59.2	56.8
Central Peak of Impact Crater North of Hellas Planitia : ESP_044952_1555 ESP_062833_1555 (Interval in Earth days: 1393)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.1	90.0	-6.3	7.712	66.7	67.7
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