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

Isolated Dune Field in Crater Northwest of Syrtis Major Planum: ESP_087903_2050 ESP_089050_2050 (Interval in Earth days: 90)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.85	71.6	-17.	0.922	45.3	47.0
Crater with Evidence of Glacial Erosion: ESP_087913_2160 ESP_088124_2160 (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
35.79	156.	-6.9	-20.2	43.2	44.7
Topographic and Albedo Feature in Western Arcadia Planitia: ESP_087873_2190 ESP_088308_2190 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.78	167.	-3.9	13.58	42.9	41.9
Kasei Valles Scarps and Terraces: ESP_087921_2055 ESP_087855_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
25.07	301.	-29.	-8.33	46.5	44.4
Layering in Sinuous Terrain: ESP_087886_1715 ESP_088176_1715 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.40	178.	-8.3	8.079	59.4	59.5
North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_087725_2165 ESP_087659_2165 (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
36.39	248.	-8.9	6.861	43.1	41.7
Crater near Marte Vallis: ESP_087701_1980 ESP_088268_1980 (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
17.73	184.	6.84	-6.87	44.6	47.5
Small Delta or Fan: ESP_087771_2065 ESP_087837_2065 (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
26.42	74.2	-7.4	-23.7	43.8	45.4
Layering in Western Lucus Planum: ESP_087912_1725 ESP_087978_1725 (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
-7.58	187.	5.90	-20.6	58.1	60.2
Terrain East of Schiaparelli Crater: ESP_087773_1770 ESP_088485_1770 (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
-2.90	22.3	4.38	-6.57	54.7	57.8
	Page 29 of 881 (8,805 images)