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

Channels and Streamlined Landforms: ESP_017666_1935 ESP_017732_1935 (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
13.13	169.	9.37	-13.0	46.2	48.1
Impact Crater Exposing Stratigraphy in Eos Chasma: ESP_017463_1630 ESP_018241_1630 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-16.6	315.	4.08	-7.28	63.1	65.0
Unnamed Crater on Rim of Valles Marineris: ESP_017556_1650 ESP_018268_1650 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.7	297.	-12.	0.635	63.2	63.2
Well-Preserved Impact Crater in Tempe Terra: ESP_017345_2200 ESP_017846_2200 (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
39.72	291.	-6.3	7.647	41.8	41.2
Possible Kieserite Deposit on Flanks of Hebes Mensa: ESP_017319_1785 ESP_017385_1785 (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
-1.24	284.	10.7	-13.0	52.2	54.2
Volcanic Rootless Constructs in the Western Tartarus Colles: ESP_017389_2070 ESP_017890_2070 (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
26.51	171.	-9.2	7.114	42.8	42.5
Gully Landforms in Aram Chaos: ESP_017528_1830 ESP_018596_1830 (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
2.770	339.	-6.7	15.40	52.0	51.9
Polygonal Ridges : ESP_017348_1910 ESP_018548_1910 (Interval in Earth days: 93)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.78	212.	3.20	-21.0	46.7	51.2
Pits along Fractures in Crater Floor Material: ESP_017103_2255 ESP_018092_2255 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.98	57.3	-5.1	-18.6	42.6	44.8
Light-Toned Rocks inside a Crater: ESP_017292_1680 ESP_025375_1680 (Interval in Earth days: 630)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.8	304.	-4.3	26.62	59.6	50.6
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