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

Olympus Mons: ESP_081700_1980 ESP_081634_1980 (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
17.84	227.	4.55	24.18	57.6	55.6
Hillslope Morphologies near Holden Crater: ESP_081723_1550 ESP_082000_1550 (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
-24.7	325.	-8.5	-22.2	64.3	63.1
The Oldest Sedimentary Rocks on Mars: ESP_049832_1560 ESP_049898_1560 (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
-23.9	57.3	-1.5	-19.2	32.8	34.7
Southern Canyon Wall in East Coprates Chasma: ESP_081605_1640 ESP_081671_1640 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.6	304.	7.52	-13.4	60.9	62.2
Inverted Features and Layers South of Moreux Crater: ESP_081667_2190 ESP_081812_2190 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.84	44.8	4.81	19.82	61.4	62.1
Mass Movement Chutes: ESP_081407_1640 ESP_081552_1640 (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
-15.8	309.	3.14	21.12	62.2	60.1
Shallow Raised-Rimmed Depression with Lobate Margin: ESP_081669_2165 ESP_081814_2165 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.13	350.	3.35	19.09	60.8	61.4
Well-Preserved 15-Km Impact Crater: ESP_081590_1700 ESP_082223_1700 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.66	353.	7.67	22.76	59.3	56.1
Glaciers and Ridges: ESP_081561_2135 ESP_081706_2135 (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
33.10	60.3	-4.8	11.17	59.4	59.8
Ridged Flow-Like Features in Deuteronilus Mensae: ESP_081694_2225 ESP_081549_2225 (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
42.00	26.9	7.78	-5.93	62.5	61.6
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