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

Intersecting Graben in Olympus Mons Aureole: ESP_016965_2035 ESP_017110_2035 (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
23.07	228.	-6.9	5.601	42.2	41.6
Depression and Small Cone with Summit Depression amid Flows: ESP_016942_1845 ESP_018010_1845 (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
4.627	138.	-6.8	7.884	48.3	51.1
Crater in Southeastern Sinus Meridiani: ESP_017250_1710 ESP_018885_1710 (Interval in Earth days: 128)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-9.04	10.7	-3.2	15.66	57.6	57.7
Channels in Tharsis Region: ESP_017281_2005 ESP_017426_2005 (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
20.48	241.	-11.	2.375	44.0	43.4
Light-Toned Mounds in Ganges Chasma: ESP_017173_1715 ESP_018518_1715 (Interval in Earth days: 105)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.40	313.	-7.9	-19.4	57.0	60.4
Crater Rim and Ejecta in Olympus Mons Aureole: ESP_017295_2050 ESP_017440_2050 (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
24.54	218.	-3.9	8.729	42.5	41.8
Exposure of North Polar Layered Deposits: ESP_017106_2670 ESP_071530_2670 (Interval in Earth days: 4240)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.18	267.	0	-6.89	64.3	65.6
Polygonal Cracks inside a Crater: ESP_017090_2475 ESP_017525_2475 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
67.17	47.8	-6.5	7.758	51.5	49.1
Eastern Portion of Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_017101_1810 ESP_017312_1810 (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
0.766	116.	7.04	-2.87	50.2	52.0
Light-Toned Mounds in Acidalia Planitia: ESP_017132_2250 ESP_017633_2250 (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
44.43	345.	-6.6	5.659	42.7	41.6
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