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

Channel in Margaritifer Terra: ESP_035949_1685 ESP_043571_1685 (Interval in Earth days: 594)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.4	345.	-7.7	18.29	62.1	55.4
Echus Montes: ESP_035938_1900 ESP_036993_1900 (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
9.935	281.	9.98	-19.3	49.4	54.5
Well-Preserved Impact Crater: ESP_035681_1920 ESP_043158_1920 (Interval in Earth days: 583)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.75	98.0	2.69	16.07	48.6	41.0
Inverted Channel Deep within Crater in Aeolis Dorsa: ESP_035600_1765 ESP_061090_1765 (Interval in Earth days: 1986)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-3.38	151.	2.24	22.85	56.3	49.3
Evidence of Ice and Rock in Crater Near Side Channel of Mamers Valles: ESP_035618_2175 ESP_036884_2175 (Interval in Earth days: 99)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.14	15.1	-2.5	-22.5	42.8	53.2
Eastern Side of Terraced Deltaic Fan in Coprates Catena Trough: ESP_035832_1650 ESP_052368_1650 (Interval in Earth days: 1289)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.0	299.	-6.3	-22.2	64.3	59.4
Exposure of North Polar Layered Deposits at Cap Edge: ESP_035963_2610 ESP_036003_2610 (Interval in Earth days: 3)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
80.83	296.	2.27	-16.7	58.7	60.2
Terraced Mesas in Mamers Valles: ESP_035697_2195 ESP_035763_2195 (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
39.24	16.8	8.52	-7.04	42.1	43.7
South Kasei Valles Flow Front: ESP_035647_2065 ESP_036913_2065 (Interval in Earth days: 98)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
26.27	304.	6.69	-18.1	43.4	52.3
Candidate Future Landing Site: ESP_035640_1845 ESP_036906_1845 (Interval in Earth days: 99)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.369	136.	25.8	-1.78	50.3	54.2
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