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

Central Peak and Floor of Large Crater West of Schiaparelli Crater: PSP_007822_1775 PSP_008178_1775 (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
-2.30	11.7	2.98	-8.20	49.3	52.9
Hematite in West Candor Chasma: PSP_007601_1745 PSP_010449_1745 (Interval in Earth days: 222)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.55	286.	7.08	-20.0	48.5	59.7
Central Peak and Interior of Large Fresh Gullied Crater: PSP_007757_2190 ESP_016618_2190 (Interval in Earth days: 691)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
38.65	341.	0.54	-21.6	42.0	43.7
Central Pit of Large Crater South of Valles Marineris: PSP_007047_1640 PSP_010264_1640 (Interval in Earth days: 251)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.9	296.	-7.3	5.642	48.3	63.0
Light-Toned Rock Exposures: PSP_007101_1730 ESP_019311_1730 (Interval in Earth days: 952)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.99	260.	-7.9	3.361	44.7	56.7
Possible Sulfates in Coprates Chasma: PSP_007205_1660 ESP_024505_1660 (Interval in Earth days: 1348)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.9	301.	5.58	-16.3	48.4	44.1
Cones and Pitted Material Inside An Embayed Crater in the Tartarus Montes: PSP_007605_2055 PSP_007961_2055 (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
25.39	173.	4.99	-5.25	40.0	41.8
Etched Terrain with Possible Layering West of Juventae Chasma: PSP_007482_1760 PSP_009486_1760 (Interval in Earth days: 156)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.20	296.	1.06	-9.01	47.0	58.5
Layering in Uzer Crater Wall Seen in MOC Image E01-00244: PSP_008073_1785 PSP_009721_1785 (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
-1.27	358.	-2.0	13.86	51.2	55.4
Fractured Terrain in Elysium Planitia: PSP_007711_1870 PSP_008067_1870 (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
6.775	161.	7.20	-4.18	43.9	47.3
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