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

Ejecta of Crater Sectioned by Erosion: ESP_013362_1710 ESP_013784_1710 (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
-8.89	315.	6.60	-9.43	42.6	38.8
Comparative Gully Morphology: ESP_013934_1335 ESP_014000_1335 (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
-46.0	183.	6.35	-11.3	40.0	41.5
Layering in Argyre Planitia Sinuous Ridge: ESP_012927_1245 ESP_013626_1245 (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
-55.1	318.	1.77	-23.3	48.2	46.0
Contact between Wallrock and Light-Toned Deposits in Hebes Chasma: ESP_013772_1795 ESP_022910_1795 (Interval in Earth days: 712)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.51	283.	-21.	-5.7	43.5	37.1
Differential Erosion of Light-Toned Stratigraphy in Melas Chasma: ESP_013640_1710 ESP_012928_1710 (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
-8.93	285.	8.51	-10.3	39.1	48.9
Gullies in Southern Hemisphere Crater: ESP_013749_1410 ESP_013894_1410 (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
-38.8	195.	-16.	-5.65	38.5	37.6
Basal Exposure of South Polar Layered Deposits: ESP_013290_1075 ESP_013092_1075 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-72.2	138.	-18.	5.428	55.8	55.0
Recent 10 Kilometer Diameter Crater in Ares Vallis: ESP_013335_1975 ESP_020772_1975 (Interval in Earth days: 580)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.40	329.	1.40	17.37	58.3	58.8
Northwest Wall of Juventae Chasma: ESP_013244_1760 ESP_030228_1760 (Interval in Earth days: 1323)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.14	296.	0	10.99	46.6	50.0
Layered Bedrock on the Floor of an Impact Crater: ESP_012881_1880 ESP_013158_1880 (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
8.116	125.	0.85	-24.8	56.6	55.9
	Page 714 of 862 (8,618 images)