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

Hydrated Materials in Columbus Crater: ESP_077218_1505 ESP_077640_1505 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-29.2	193.	0	23.47	51.7	56.7
Mesa near Mawrth Vallis: ESP_077450_2055 ESP_077951_2055 (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
25.02	336.	-8.9	3	42.3	41.5
Crater in Arabia Terra: ESP_077251_2150 ESP_077528_2150 (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
34.54	5.36	-7.6	1.733	46.5	44.3
Channel in Terra Cimmeria: ESP_077481_1415 ESP_086355_1415 (Interval in Earth days: 692)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.4	217.	6.91	28.75	61.4	60.7
Glacial Flow into Crater Central Pit: ESP_077127_2150 ESP_076718_2150 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.80	150.	-18.	-0.45	48.3	50.7
Recent Crater: ESP_077370_2130 ESP_077858_2130 (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
32.80	357.	-2.7	-25.4	44.7	45.2
Alluvial Fan in Kasei Valles: ESP_077148_2035 ESP_084809_2035 (Interval in Earth days: 597)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.42	296.	0.66	22.69	41.6	50.3
Hebes Chasma Layers: ESP_077241_1790 ESP_085258_1790 (Interval in Earth days: 625)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.80	282.	-5.3	15.27	40.2	34.7
Origin of Channels in Southern Low-Latitudes: ESP_077368_1685 ESP_078080_1685 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.2	58.0	-5.7	10.09	44.8	52.5
Ejecta of Well-Preserved 12-Kilometer Impact Crater in South Utopia Planitia: ESP_077194_2070 ESP_077260_2070 (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
26.82	120.	4.00	-7.09	42.5	43.1
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