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

Ridge Over Hill in Hellas Planitia: ESP_086821_1375 ESP_086676_1375 (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
-41.9	97.7	-3.9	-15.1	72.1	70.7
High-Latitude Crater: ESP_086952_2425 ESP_088099_2425 (Interval in Earth days: 90)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
62.05	104.	3.58	29.37	52.9	45.4
Channeled Terraces and Debris Fan in Crater in Arabia Terra: ESP_087022_2165 ESP_087167_2165 (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
35.93	0.65	-9.7	3.05	43.4	42.1
Pitted Cone with Clear Moat: ESP_086926_2080 ESP_087071_2080 (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
27.85	102.	-8.9	4.814	42.3	41.3
Hillslope Morphologies near Murray Crater: ESP_087074_1555 ESP_087219_1555 (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
-24.0	28.1	-7.1	10.08	63.0	63.5
Small Shield Volcano East of Ascraeus Mons: ESP_087118_1920 ESP_087606_1920 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.96	261.	5.03	-20.6	43.8	48.5
Small Alluvial Fans in Kasei Valles: ESP_087156_2065 ESP_087011_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
26.44	299.	26.2	13.41	39.5	40.5
Layers and Features in Arabia Terra Crater: ESP_087100_1860 ESP_087667_1860 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
6.225	34.5	-6.5	7.77	46.6	49.1
Light-Toned Deposits in Arsinoes Chaos: ESP_086865_1720 ESP_087709_1720 (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
-8.10	331.	-3.0	-16.6	50.8	58.9
Northern Plains Crater: ESP_086922_2295 ESP_087199_2295 (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
49.01	208.	-5.1	-21.0	47.3	47.4
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