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

Well-Preserved 30-Kilometer Impact Crater: ESP_039176_1615 ESP_039387_1615 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.5	98.5	6.16	-4.52	47.3	45.5
Well-Preserved 2-Kilometer Crater over Bedrock: ESP_039138_1545 ESP_046852_1545 (Interval in Earth days: 601)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.4	58.0	-6.0	9.496	47.7	53.8
Well-Preserved Impact Crater on Floor of Coprates Chasma: ESP_039182_1675 ESP_048465_1675 (Interval in Earth days: 723)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.3	294.	-4.8	7.502	49.6	39.1
Margin of Pedestal Crater in Malea Planum: ESP_039126_1215 ESP_039627_1215 (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
-58.3	31.4	-5.5	7.724	53.2	46.8
Candidate ExoMars Landing Site: ESP_039036_1925 ESP_039458_1925 (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
12.14	315.	26.1	6.489	58.6	57.6
Landforms of Eastern Hydraotes Chaos: ESP_039128_1800 ESP_039761_1800 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.16	327.	1.77	-15.4	54.0	48.9
Flow Features in Arimanes Rupes Region East of Mangala Valles: ESP_038908_1670 ESP_039396_1670 (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
-12.7	212.	26.6	-4.87	49.7	47.0
Pavonis Mons: ESP_039131_1830 ESP_039342_1830 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.876	244.	6.87	-5.46	55.0	54.2
Double Crater with Flow Features on Floor: ESP_038946_1780 ESP_039447_1780 (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
-1.87	257.	-16.	4.971	55.9	50.2
Osuga Valles Lowest Point: ESP_039181_1650 ESP_039326_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	322.	-5.4	7.662	49.0	46.3
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