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

Candidate ExoMars Landing Site: ESP_039299_1985 ESP_047501_1985 (Interval in Earth days: 639)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.21	335.	6.94	-19.6	62.4	60.7
Proposed Landing Site for ExoMars Rover at Aram Dorsum: ESP_039470_1880 ESP_039536_1880 (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
7.960	348.	8.22	-13.5	54.9	55.8
Small Cone in Hydraotes Chaos: ESP_039550_1805 ESP_039484_1805 (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
0.465	326.	-10.	11.74	51.3	50.4
Impact Crater into Side of Massif: ESP_039230_1545 ESP_039375_1545 (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
-25.3	66.0	-4.9	8.63	46.4	43.4
Beagle 2 Lander Credible Candidate: ESP_039519_1915 ESP_040363_1915 (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
11.51	90.4	4.3	-15.9	56.9	48.4
Cones on Crater Floor in Terra Sirenum: ESP_039370_1520 ESP_066152_1520 (Interval in Earth days: 2087)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.6	203.	3.99	27.94	43.6	39.7
Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_039203_1985 ESP_039348_1985 (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
18.24	77.8	-5.7	6.917	63.6	62.1
Flows Near Echus Chasma: ESP_039222_1865 ESP_040066_1865 (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
6.218	279.	2.15	-19.2	56.3	49.0
Debris Apron and Flow Features in Reull Vallis: ESP_039519_1400 ESP_039018_1400 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.4	96.0	13.1	0	41.4	49.3
Pits in Hale Crater Ejecta: ESP_039524_1445 ESP_039801_1445 (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
-35.0	320.	-2.4	-19.2	42.0	40.3
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