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

Inverted Valley and Rings in Erebus Montes: ESP_089718_2210 ESP_090061_2210 (Interval in Earth days: 26)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.86	188.	26.6	-1.13	49.3	55.9
Planned ExoMars Landing Site in Oxia Planum: ESP_089726_1975 ESP_089225_1975 (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
17.14	336.	11.0	-14.0	50.8	50.8
Large Alluvial Fan in Kasei Valles: ESP_089846_2065 ESP_089991_2065 (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
26.23	300.	-2.1	14.95	51.9	51.7
Streamlined Shape and Possible Bar South of Semeykin Crater: ESP_089883_2195 ESP_090028_2195 (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
39.01	8.16	-0.2	14.06	53.3	53.8
Volcanic Cones in Ceraunius Fossae: ESP_089650_2050 ESP_089927_2050 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.57	250.	6.19	-14.8	49.8	53.6
Exposed Layers in Olympia Mensae Icy Outliers: ESP_089774_2545 ESP_089787_2545 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
74.13	95.1	-4.3	10.35	64.8	63.9
Kasei Valles Alluvial Fan and Distributary Channels: ESP_089899_2035 ESP_089622_2035 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.09	293.	-4.0	17.28	52.5	48.8
Dune Interaction with Residual Polar Ice: ESP_089800_2600 ESP_089826_2600 (Interval in Earth days: 2)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
79.64	98.5	-0.5	16.96	67.8	67.0
Glacier Layering Revealed by Impact Crater on Viscous Flow Features Surface: ESP_089764_2200 ESP_089487_2200 (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
39.61	17.6	-8.7	10.06	52.8	48.4
Kasei Valles Alluvial Fans and Flood Terrace: ESP_089820_2025 ESP_089675_2025 (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
22.03	290.	-0.2	-16.9	51.7	52.1
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