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

Cones and Pitted Material Inside An Embayed Crater in the Tartarus Montes: PSP_007605_2055 PSP_007961_2055 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.39	173.	4.99	-5.25	40.0	41.8
Etched Terrain with Possible Layering West of Juventae Chasma: PSP_007482_1760 PSP_009486_1760 (Interval in Earth days: 156)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.20	296.	1.06	-9.01	47.0	58.5
Layering in Uzer Crater Wall Seen in MOC Image E01-00244: PSP_008073_1785 PSP_009721_1785 (Interval in Earth days: 128)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.27	358.	-2.0	13.86	51.2	55.4
Fading Rayed Crater in Daedalum Planum: PSP_007735_1570 ESP_028345_1570 (Interval in Earth days: 1606)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.0	230.	2.03	-10.9	60.9	63.5
Mawrth Vallis Phyllosilicates: PSP_007019_1980 ESP_077041_1980 (Interval in Earth days: 5456)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.68	336.	0.65	16.95	38.6	38.7
Gullies on South-Facing Wall of Crater: PSP_007045_1450 ESP_016130_1450 (Interval in Earth days: 708)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.6	353.	-5.7	-23.5	59.8	64.8
Fresh Multiple-Layer-Ejecta Crater in Southern Highlands: PSP_007154_1360 ESP_019931_1360 (Interval in Earth days: 996)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.6	258.	-2.4	12.90	67.7	69.0
Light-Toned Tilted Layering in Central Peak of Oudemans Crater: PSP_007694_1700 ESP_027882_1700 (Interval in Earth days: 1574)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.92	268.	1.09	-17.4	52.3	59.3
Craters on an Ice-Rich Debris Apron: PSP_007832_1385 ESP_060736_1385 (Interval in Earth days: 4123)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-41.3	103.	1.98	-19.2	74.9	74.8
Stair-Stepped Slope Seen in MOC Image R08-00823: PSP_007684_1795 ESP_020171_1795 (Interval in Earth days: 973)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.44	180.	-5.7	17.22	47.7	53.5
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