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 and Fan System in Reuyl Crater: ESP_026079_1700 ESP_026224_1700 (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
-10.0	167.	-0.1	15.48	56.9	56.7
Well-Preserved Impact Crater in Utopia Planitia: ESP_026015_2045 ESP_026292_2045 (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
24.43	107.	27.8	4.068	38.2	41.2
Layered Light-Toned Rounded Blocks in Melas Chasma: ESP_025811_1700 ESP_026312_1700 (Interval in Earth days: 39)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.2	284.	-7.9	16.99	55.8	57.1
Flow Features in Crater Near Cerberus Fossae: ESP_025934_1905 ESP_026567_1905 (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
10.41	162.	6.71	-13.0	44.4	48.3
Furthest Part of Young Channel in Lyot Crater: ESP_025899_2295 ESP_026031_2295 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
49.20	30.5	20.2	-6.05	40.6	42.7
Flow with Wide Leveed Channel: ESP_025998_1760 ESP_027264_1760 (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
-3.90	217.	3.13	-22.8	52.5	57.3
Hellas Planitia Terrain: ESP_026083_1430 ESP_026505_1430 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.7	59.1	24.7	15.20	74.5	76.8
Gale Crater: ESP_026001_1750 ESP_027979_1750 (Interval in Earth days: 154)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.86	137.	-12.	11.95	54.1	54.7
Channel from Main Athabasca Valles Channel: ESP_025908_1875 ESP_026053_1875 (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
7.418	153.	-1.5	13.07	46.2	45.9
Impact-Induced Fan Formation in Phlegra Dorsa: ESP_025973_2030 ESP_025828_2030 (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
22.75	175.	12.6	-1.33	40.0	40.7
	Page 593 of 896 (8,955 images)