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

Contact between Polygon and Massif: PSP_005700_2200 ESP_011818_2200 (Interval in Earth days: 477)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.77	346.	0	-24.3	59.2	72.7
Xanthe Terra Crater: PSP_006598_1780 ESP_033326_1780 (Interval in Earth days: 2083)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.16	313.	2.29	24.68	37.1	37.0
Pits in Southwest Pavonis Mons: PSP_005071_1775 PSP_005783_1775 (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
-2.67	244.	-8.1	8.61	39.4	33.4
Exposure of Polar Layered Deposits within Southern Residual Cap: PSP_005029_0930 PSP_005239_0930 (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
-86.8	11.6	0.89	15.20	68.5	69.6
Gullies with Bright Color Deposits: PSP_005082_1365 ESP_012703_1365 (Interval in Earth days: 594)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.0	309.	-0.9	23.99	38.4	46.0
Layered Rock Outcrops in West Candor Chasma: PSP_005742_1750 PSP_006665_1750 (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
-4.93	285.	1.77	-8.25	33.5	39.1
Ithaca Region Defrosted: PSP_004666_0945 PSP_004891_0945 (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
-85.2	181.	-0.9	-18.0	64.2	67.5
Lobate Crater Ejecta: PSP_005867_1330 ESP_011431_1330 (Interval in Earth days: 434)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.4	118.	0	14.15	48.3	67.4
Tomini Crater Western Ejecta: PSP_005695_1965 PSP_005985_1965 (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
16.25	125.	-1.0	26.25	42.8	38.2
Streamlined Hills in the Western Charitum Montes: PSP_006902_1275 ESP_011398_1275 (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
-52.1	301.	-7.0	7.062	70.2	70.9
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