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

Central Peak Gullies: PSP_006162_1365 PSP_007085_1365 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.2	343.	0	-11.5	50.7	66.8
Geologic Contacts in Juventae Chasma: PSP_008708_1780 PSP_008998_1780 (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
-2.16	298.	-4.2	5.893	55.4	55.6
Gullies with Meandering Channels and Channels That Widen Downslope: PSP_005930_1395 PSP_006853_1395 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-40.3	196.	5.53	-8.46	44.8	60.8
Utopia Planitia Landforms: PSP_008452_2175 PSP_008663_2175 (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
37.11	82.8	7.01	-11.5	41.0	42.9
Lineated Valley Fill in Coloe Fossae: PSP_008598_2155 PSP_008954_2155 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
35.16	57.2	-3.6	-18.8	42.2	44.3
Layers in Uzboi Vallis: PSP_008338_1525 PSP_010329_1525 (Interval in Earth days: 155)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.4	324.	5.23	-10.4	69.3	70.2
Crater Floor Fan: PSP_008233_1920 PSP_008879_1920 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.72	307.	6.25	-7.44	45.5	49.1
Western Rim and Ejecta of Largest Rayed Crater Known on Mars: PSP_007949_1970 ESP_024814_1970 (Interval in Earth days: 1315)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.90	141.	-0.8	-28.1	42.9	39.9
Hellas Planitia: PSP_007913_1370 ESP_016642_1370 (Interval in Earth days: 680)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.6	52.4	1.81	18.41	76.8	74.9
Area Near Summit of Gale Crater Mound: PSP_008002_1750 PSP_009927_1750 (Interval in Earth days: 151)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.85	137.	-5.8	-22.8	52.8	59.9
	Page 771 of 862 (8,618 images)