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

Flow Lobes in Northern Plains Crater: PSP_009803_2505 PSP_009935_2505 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
70.28	266.	4.45	-8.78	54.9	57.1
Layering Under Crater Ejecta: PSP_009324_1830 ESP_020374_1830 (Interval in Earth days: 861)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.065	37.4	2.15	20	53.7	53.6
Mamers Valles: PSP_009773_2165 ESP_053789_2165 (Interval in Earth days: 3429)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.13	14.3	5.21	-4.42	45.5	42.7
Exposure of North Polar Layered Deposits for Stratigraphic Analysis: PSP_009471_2670 PSP_009683_2670 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
86.93	301.	-8.2	-21.8	63.0	65.1
Possible Flute Casts in Ares Vallis: PSP_009722_1960 PSP_009867_1960 (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
15.92	329.	2.51	17.22	48.9	48.1
Scarp-Fed Dark Dunes: PSP_009885_2655 PSP_010344_2655 (Interval in Earth days: 36)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
85.68	179.	-14.	15.88	65.5	70.3
Small Shield Covering the Noctis Fossae: PSP_010305_1780 PSP_010661_1780 (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
-1.91	256.	-7.0	-0.74	57.3	56.9
Terrain West of Hecates Tholus: PSP_009742_2150 PSP_010243_2150 (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
34.47	142.	-6.3	14.22	46.4	48.3
Irregular Craters in Olympus Mons Aureole: PSP_009818_2145 PSP_010886_2145 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.15	226.	4.26	21.63	45.9	54.5
Fresh 8-Kilometer Diameter Impact Crater: PSP_009625_1900 ESP_016060_1900 (Interval in Earth days: 501)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.793	98.5	4.97	-22.4	50.7	41.9
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