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

Well-Exposed Crater Ejecta in Tyrrhena Terra: ESP_064877_1670 ESP_064811_1670 (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
-12.9	83.0	8.74	27.89	55.5	54.1
Stratified Mound in North Oxia Colles: ESP_064683_2055 ESP_064749_2055 (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
25.06	334.	4.26	-13.9	63.9	65.9
Nicholson Crater: ESP_064530_1800 ESP_064807_1800 (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
0.058	195.	-0.4	-23.4	57.6	59.8
Sublimation at Spiders Site: ESP_064785_0930 ESP_064639_0930 (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
-87.0	127.	8.53	21.89	80.1	81.5
Valleys in Crater Northeast of Argyre Planitia: ESP_064736_1500 ESP_064591_1500 (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
-29.7	335.	0.30	-16.8	58.2	61.0
Fractures and Inlet Valley : ESP_064798_1990 ESP_064653_1990 (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
18.64	76.2	0.85	-16.8	62.7	63.1
Small Barchan Dunes in Northeast Argyre Region: ESP_064789_1350 ESP_064723_1350 (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
-44.6	331.	-5.9	10.38	61.7	61.4
Baetis Chasma: ESP_064645_1760 ESP_065410_1760 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.19	295.	8.33	-23.4	56.7	56.9
Flow Features in Reull Vallis: ESP_064837_1405 ESP_065391_1405 (Interval in Earth days: 43)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-39.4	96.2	28.3	5.137	56.8	51.1
Fan-Shaped Deposit with Floor Outcrop in Camichel Crater: ESP_064750_1825 ESP_065304_1825 (Interval in Earth days: 43)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.468	308.	4.35	-28.4	57.9	60.2
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