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

Survey Layering and Faulting in Layered Deposits in Candor Chasma: PSP_001377_1685 PSP_001852_1685 (Interval in Earth days: 37)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.3	286.	0	13.98	60.1	57.7
Light-Toned Layered Material in South Galle Crater : PSP_002866_1280 ESP_064565_1280 (Interval in Earth days: 4808)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-51.8	329.	1.76	-20.3	65.7	68.7
Pristine-Looking Gully : PSP_002692_2295 PSP_002824_2295 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
49.13	25.2	5.98	-20.2	69.2	73.3
Blocks in the Olympus Mons : PSP_003450_1975 ESP_012060_1975 (Interval in Earth days: 671)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.42	216.	2.71	26.11	61.9	60.8
Possible Cinder Cone on the Southern Flank of Pavonis Mons: PSP_002671_1790 ESP_011413_1790 (Interval in Earth days: 681)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.10	246.	-2.3	-18.2	55.8	58.8
Sand Dunes in Rabe Crater: PSP_002824_1355 PSP_003325_1355 (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
-43.9	34.5	4.86	26.51	63.0	53.6
Candidate Cavern Entrance Northeast of Arsia Mons: PSP_003647_1745 PSP_004847_1745 (Interval in Earth days: 94)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.53	241.	-0.5	-16.3	52.3	41.1
Very Fine Layers in Juventae Chasma: PSP_002590_1765 PSP_002946_1765 (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
-3.29	298.	-2.1	6.197	55.9	54.9
Evros Vallis and Nearby Craters: PSP_003273_1675 PSP_003695_1675 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.6	13.3	-6.9	-18.2	53.7	51.3
Dark Slope Streak with Streak-Generated Topography: PSP_003542_2035 PSP_005599_2035 (Interval in Earth days: 160)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.32	223.	7.06	20.76	64.9	47.3
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