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

Potential Rhythmic Layering in East Gale Crater with Hydrated Signature: ESP_016375_1750 ESP_016520_1750 (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
-5.15	138.	1.01	18.09	48.0	48.2
Olivine-Rich Terrain in Yuty Crater: ESP_016579_2025 ESP_017647_2025 (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
22.08	325.	1.00	18.99	40.6	42.1
Crater with Lineated Material on Floor: ESP_016824_1465 ESP_016969_1465 (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
-33.2	124.	-2.9	10.86	71.0	71.5
Very Well-Preserved 12-Kilometer Diameter Crater: ESP_016569_2320 ESP_016846_2320 (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
51.40	234.	-1.5	-15.9	46.0	46.1
25-Kilometer Diameter Gullied Impact Crater in Acidalia Planitia: ESP_016592_2170 ESP_016737_2170 (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
36.54	329.	-3.7	9.38	41.6	40.3
Possible Phyllosilicate-Rich Area in Syrtis Major: ESP_016628_2040 ESP_017340_2040 (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
23.69	68.6	-7.2	6.233	41.2	42.0
Fretted Valley Outlet: ESP_016391_2195 ESP_016668_2195 (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
38.96	56.1	-0.8	-19.4	42.2	43.3
Small Crater Exposed in Cross-Section by Erosion: ESP_016699_1715 ESP_019178_1715 (Interval in Earth days: 193)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.45	293.	1.41	-13.7	52.9	58.8
Gordii Dorsum: ESP_016847_1910 ESP_017559_1910 (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
10.61	211.	-2.9	6.107	44.9	47.3
Crater Superposed on Mamers Vallis Seen in MOC Image R1802279: ESP_016366_2125 ESP_016511_2125 (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
31.95	18.7	8.24	20.96	40.0	38.7
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