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

Mounds on Kashira Crater Floor: ESP_011370_1525 ESP_029053_1525 (Interval in Earth days: 1378)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.1	341.	8.46	-10.0	61.4	59.8
Very Fresh 1-Kilometer Impact Crater: ESP_011563_2200 ESP_011853_2200 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.70	104.	4.18	26.78	66.9	68.9
Large Channel Emanating from Summit of Ceraunius Tholus: ESP_011399_2045 PSP_006191_2045 (Interval in Earth days: 406)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.18	262.	16.5	0	58.8	42.8
Western Half of Very Fresh Crater in Utopia Region: PSP_010402_2050 ESP_053495_2050 (Interval in Earth days: 3357)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
24.57	124.	-2.7	-23.1	51.1	44.1
Outcrops of Light-Toned Materials Exposed in Highlands Crater Wall: PSP_010448_1530 ESP_016751_1530 (Interval in Earth days: 491)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.7	315.	-5.7	11.67	68.8	64.8
Fresh Impact Crater on Northern Plains: PSP_010441_2385 PSP_010810_2385 (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
58.19	135.	-7.9	20.93	58.0	61.1
Possible Active Geyser Locale: ESP_011406_0945 ESP_011407_0945 (Interval in Earth days: 0)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-85.4	103.	14.4	-9.73	87.5	89.6
Light-Toned Layering along Wallrock in Southwest Melas Chasma: ESP_011504_1700 ESP_016106_1700 (Interval in Earth days: 359)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.99	284.	-28.	-15.4	60.3	48.7
Crater Wall in Chryse Planitia: PSP_010408_2070 ESP_045906_2070 (Interval in Earth days: 2766)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
26.88	319.	2.47	-6.79	50.6	48.1
Crater with Extensive Ejecta Deposits: PSP_010611_2210 ESP_027173_2210 (Interval in Earth days: 1290)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.51	175.	0.50	-12.9	54.2	44.1
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