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

Coprates Chasma Wall: PSP_007218_1660 PSP_010712_1660 (Interval in Earth days: 273)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.1	306.	-0.3	-14.9	49.1	62.2
Small But Very Deep Pit North of Arsia Mons: PSP_007774_1745 PSP_008130_1745 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.30	242.	6.40	-5.72	50.2	54.0
Central Peak of Fesenkov Crater: PSP_007931_2020 ESP_024585_2020 (Interval in Earth days: 1298)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.68	273.	-8.3	-25.5	42.4	39.6
Western Portion and Ejecta of Well-Preserved Crater: PSP_007804_1970 PSP_009307_1970 (Interval in Earth days: 117)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.91	141.	-5.6	-18.2	42.5	49.1
Landforms of the Aeolis and Zephyria Regions: PSP_007606_1785 ESP_016190_1785 (Interval in Earth days: 669)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.38	150.	-1.3	-16.7	47.1	45.8
Ring and Cone Structures in Grjota Valles: PSP_007869_1960 PSP_007579_1960 (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
15.90	164.	18.0	4.908	41.1	40.7
Unnamed Small Rayed Crater in Hesperia Region: PSP_008135_1520 PSP_008425_1520 (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
-27.9	108.	-4.0	6.037	68.6	70.2
Olympus Mons North Scarp Detail: PSP_007735_2030 PSP_008091_2030 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.92	224.	4.41	-5.92	40.5	42.5
Western Rim and Ejecta of Largest Rayed Crater Known on Mars: PSP_007949_1970 ESP_024814_1970 (Interval in Earth days: 1315)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.90	141.	-0.8	-28.1	42.9	39.9
Center of Mars: PSP_007361_1800 ESP_041909_1800 (Interval in Earth days: 2692)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.01	0.00	-0.1	20.55	44.1	35.7
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