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

Domoni Crater Secondaries: ESP_034832_2300 ESP_035887_2300 (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
49.69	231.	0.40	-18.2	43.0	46.5
Channels on Mesa in Southern Elysium Planitia: ESP_034558_1775 ESP_052307_1775 (Interval in Earth days: 1383)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.48	159.	6.18	26.96	50.8	47.7
Sinuous Ridge with Mesa at Terminus in Kasabi Crater: ESP_034508_1520 ESP_035154_1520 (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
-27.7	89.1	-6.1	19.81	67.4	70.3
Depression with Concentric Features: ESP_034772_1515 ESP_052297_1515 (Interval in Earth days: 1366)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.4	80.7	-1.9	-25.0	69.8	68.6
Gullies: ESP_034618_2280 ESP_036530_2280 (Interval in Earth days: 149)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
47.62	315.	0.53	9.725	42.9	48.5
Low Albedo Slopes along Coprates Chasma Ridge: ESP_034619_1670 ESP_034830_1670 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.9	295.	6.13	-6.21	57.6	59.8
Crater Among Pits on Northern Plains: ESP_034647_2305 ESP_034924_2305 (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
50.11	241.	7.14	-13.6	43.0	44.3
Small Crater with Faded Rays: ESP_034854_1870 ESP_036911_1870 (Interval in Earth days: 160)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.076	357.	1.36	24.51	48.1	51.3
Fractured Surface in Avernus Region: ESP_034505_1770 ESP_034795_1770 (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
-2.74	167.	-3.6	20.02	51.2	51.6
Lava Textures inside Kasei Valles: ESP_034724_2065 ESP_035568_2065 (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
26.17	303.	4.53	-23.0	41.0	45.8
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