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

Low Shield Cut By Graben Near Ceraunius Fossae: PSP_009382_2090 ESP_016028_2090 (Interval in Earth days: 518)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
28.73	250.	0.12	-28.6	44.7	42.8
Dry Cataracts in Athabasca Valles: PSP_009702_1900 PSP_009847_1900 (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
9.873	156.	0.40	15.92	51.2	50.3
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
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
Exposure of Light-Toned Layering along Wallrock in Coprates Chasma: PSP_009684_1695 PSP_010396_1695 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-10.2	290.	-2.2	19.86	61.5	58.8
Flow on Floor of Kasei Valles: PSP_010000_2055 ESP_069104_2055 (Interval in Earth days: 4605)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.17	299.	0	22.72	48.1	44.8
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
Light-Toned Deposits and Possible Fluvial Channels on Floor of Ius Chasma: PSP_010146_1720 PSP_010568_1720 (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
-7.96	277.	-4.7	-18.8	59.9	60.5
High-Latitude Exposure of North Polar Layered Deposits: PSP_009309_2725 PSP_009589_2675 (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
87.52	327.	-4.7	-14.4	64.2	64.4
Central Peak of Crater: PSP_009561_2325 PSP_010260_2325 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
52.40	39.8	0.54	-21.0	46.6	54.9
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