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

Impact Crater adjacent to Ravine: ESP_068867_1985 ESP_078823_1985 (Interval in Earth days: 776)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.09	288.	1.03	12.18	45.8	44.6
Modification of Small Terraced Crater: ESP_068829_2480 ESP_069251_2480 (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
67.82	233.	4.32	25.32	62.9	57.0
Very Well-Preserved 900-Meter Northern Plains Crater : ESP_068700_2420 ESP_068687_2420 (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
61.49	155.	-0.2	-26.2	60.9	63.1
Cones in Tharsis Region: ESP_068895_1890 ESP_069093_1890 (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
9.120	243.	26.6	2.819	44.7	48.4
Shalbatana Vallis: ESP_068800_1855 ESP_069829_1855 (Interval in Earth days: 80)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.510	316.	4.43	-9.93	46.6	55.9
Crater Gullies at Multiple Elevations: ESP_067299_1435 ESP_067708_1435 (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
-36.1	227.	-6.6	3.913	42.9	47.4
Jezero Crater Inlet Valley : ESP_068162_1990 ESP_067159_1990 (Interval in Earth days: 78)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.66	76.6	-7.4	27.38	45.0	48.8
Pyramus Fossae: ESP_068149_2310 ESP_077130_2310 (Interval in Earth days: 700)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
50.41	66.2	-3.9	-16.6	60.2	57.4
Crater in Arabia Terra: ESP_068336_2245 ESP_069075_2245 (Interval in Earth days: 57)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.10	6.10	4.50	28.14	54.1	47.6
Chain of Layered Mounds in Chryse Planitia: ESP_068179_2000 ESP_072663_2000 (Interval in Earth days: 350)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.60	332.	-4.3	21.53	45.1	53.6
	Page 180 of 878 (8,771 images)