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

Channels and Noachian Crater Fill: ESP_012709_1445 ESP_013197_1445 (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
-35.2	146.	1.58	-27.4	46.6	42.6
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
Faulting in South Polar Layered Deposits: ESP_012762_1070 ESP_013171_1070 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-72.9	146.	10.3	-12.8	58.0	56.3
Rayed Crater: ESP_013955_1020 ESP_013968_1020 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-77.8	345.	-6.7	7.228	62.3	61.6
Crossing Wrinkle Ridges in Tyrrhena Dorsa: ESP_012631_1555 PSP_005234_1555 (Interval in Earth days: 576)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.1	115.	-1.3	17.00	48.2	31.9
Cratered Cones in Galaxias Colles: ESP_012946_2165 ESP_013236_2165 (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
36.17	147.	4.76	26.24	74.0	71.2
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
Marte Vallis Streamlined Landforms: ESP_014092_1955 ESP_014158_1955 (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
15.46	183.	-6.8	-25.9	48.1	48.6
Warrego Valles Headwater Region: ESP_013153_1390 ESP_013298_1390 (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
-40.6	266.	-5.4	6.316	42.0	39.7
Western Slope of Asimov Crater: ESP_013110_1325 ESP_013611_1325 (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
-47.0	4.17	-23.	-7.91	45.4	41.0
	Page 714 of 877 (8,766 images)