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

Barchan to Sand Sheet Transition in Central Herschel Crater: ESP_089892_1655 ESP_090037_1655 (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
-14.1	129.	-3.4	17.28	62.1	60.1
Avalanche Scarp: ESP_089821_2640 ESP_089848_2640 (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
83.78	237.	-3.9	-21.3	70.6	72.2
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
Light-Toned Exposures on Floor of Coprates Chasma: ESP_089780_1645 ESP_090057_1645 (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
-15.2	306.	6.84	-14.8	62.3	62.9
Antoniadi Crater Fluvial Features: ESP_089868_2015 ESP_089934_2015 (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
21.20	57.4	26.6	9.6	49.7	51.7
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
Scarp Contact: ESP_089889_1920 ESP_090166_1920 (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
11.85	207.	1.64	-17.1	53.2	56.1
Moraine-Like Assemblage Exposed by Ice Retreat: ESP_089855_2215 ESP_090422_2215 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.98	51.3	6.63	23.73	52.7	58.7
Features around Crater in Terra Sabaea: ESP_089842_2165 ESP_089565_2165 (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
36.09	50.5	-24.	-6.66	54.5	50.2
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