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

Terminal Lobes of Landslide or Large Debris Flow in Melas Chasma: ESP_047450_1685 ESP_048953_1685 (Interval in Earth days: 117)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.1	290.	-2.4	15.23	49.3	33.6
Well-Preserved 10-Kilometer Impact Crater: ESP_047444_2095 ESP_065193_2095 (Interval in Earth days: 1383)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
29.40	89.0	-5.8	28.88	65.3	67.9
Layers in Crater Southwestern Arabia Terra: ESP_047421_1890 ESP_064036_1890 (Interval in Earth days: 1295)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.862	-0.8	0.83	18.37	54.8	54.4
Impact Crater North of Hellas Region: ESP_047590_1520 ESP_048658_1520 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.5	68.8	5.92	-13.0	46.7	35.3
Crater in Arabia Terra: ESP_047446_1900 ESP_065393_1900 (Interval in Earth days: 1398)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.647	36.3	2.18	-7.22	55.0	61.2
Fresh Rayed Crater on Slope into Hadriaca Patera: ESP_047576_1500 ESP_048723_1500 (Interval in Earth days: 90)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-29.4	92.3	-4.4	10.48	47.8	32.9
Light-Toned Inverted Terrain in Gorgonum Chaos Basin: ESP_047546_1410 ESP_048469_1410 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.5	190.	20.9	-5.01	47.7	37.5
Two-Kilometer Diameter Rayed Crater: ESP_047484_1855 ESP_048987_1855 (Interval in Earth days: 117)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.491	79.6	-0.8	16.80	53.6	41.9
Polygonal Shapes Southwest of Olympus Mons: ESP_047611_1915 ESP_048046_1915 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.49	211.	0	27.88	56.2	53.4
Candidate ExoMars Landing Site in Oxia Palus Region: ESP_047435_1985 ESP_064195_1985 (Interval in Earth days: 1306)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.05	335.	-0.4	28.08	59.0	55.2
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