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

Crater Floor : ESP_059613_1405 ESP_067407_1405 (Interval in Earth days: 607)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.9	158.	0.61	12.76	55.4	44.0
Scarps in Icaria Region : ESP_059716_1425 ESP_059993_1425 (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
-37.1	227.	-3.5	-24.4	56.1	61.8
High-Latitude Gullies : ESP_059507_1300 ESP_059573_1300 (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
-49.8	173.	8.13	-7.77	61.4	63.3
Possible Phyllosilicate-Rich Stratigraphy in Western Mawrth Vallis: ESP_059738_2050 ESP_060094_2050 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.53	338.	-7.4	5.422	38.1	36.8
Mass Wasting Feature on Southern Wall of Crater Near Amazonis Mensa : ESP_059611_1860 ESP_060244_1860 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.755	207.	5.84	-4.61	33.9	39.7
Potential Well-Exposed Ejecta Southwest of Crater West of Ganges Chasma : ESP_059568_1720 ESP_059713_1720 (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
-8.14	302.	6.09	22.86	36.4	36.8
Craters : ESP_059632_1470 ESP_060199_1470 (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
-32.5	-0.9	2.00	12.09	51.1	59.5
Osuga Valles Depression Eastern Rim : ESP_059686_1650 ESP_059620_1650 (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
-14.7	322.	-2.4	19.52	41.4	38.9
Layers around Mound in Northern Mid-Latitudes : ESP_059709_2250 ESP_069034_2245 (Interval in Earth days: 726)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.83	47.5	-5.3	10.52	48.2	49.6
Smooth Area in Phlegra Montes : ESP_059507_2155 ESP_058795_2155 (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
35.23	163.	-7.6	-17.5	44.3	52.6
	Page 265 of 891 (8,901 images)