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

A Volcanic Pit Chain and Dust Avalanches : ESP_026249_2025 ESP_026750_2025 (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
22.26	202.	-7.3	17.82	42.6	41.8
Layered Deposits on a Crater Floor: ESP_026091_1920 ESP_026025_1920 (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
11.77	198.	-14.	7.613	46.2	44.2
Uplifted Terrain in Northern Amazonis Planitia: ESP_026011_2185 ESP_026855_2185 (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
38.01	216.	8.27	-8.29	39.3	42.2
Well-Preserved 6-Kilometer Impact Crater Near Tinjar Valles: ESP_025843_2170 ESP_026898_2170 (Interval in Earth days: 82)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.87	124.	1.11	-19.9	39.8	43.4
Cratered Cones within a Flow along Cerberus Fossae: ESP_026158_1945 ESP_026303_1945 (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
14.14	166.	7.85	21.87	43.8	43.1
Fresh 1-Kilometer Impact Crater in Arcadia Planitia: ESP_025801_2185 ESP_025735_2185 (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
38.15	191.	-6.6	8.468	40.6	39.3
Rootless Cone Intersecting Crater Rim: ESP_026170_1990 ESP_026236_1990 (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
18.94	197.	17.7	-2.54	41.2	43.1
Streamlined Landforms in Tinjar Valles: ESP_025988_2165 ESP_026067_2165 (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
36.37	126.	-2.8	24.21	40.1	37.7
Field of Transverse Aeolian Ridges with Superposed Impact Craters: ESP_025966_1765 ESP_026889_1765 (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
-3.32	12.8	-16.	0.66	53.2	55.2
Channel and Fan System in Reuyl Crater: ESP_026079_1700 ESP_026224_1700 (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
-10.0	167.	-0.1	15.48	56.9	56.7
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