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

Exposure of Thick Layered Deposits in Hebes Chasma: ESP_013205_1790 ESP_021565_1790 (Interval in Earth days: 651)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.82	283.	-25.	-3.43	50.5	51.4
Eastern Tooting Crater Impact Processes: ESP_013735_2035 ESP_014157_2035 (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
23.18	207.	6.42	-8.32	57.4	52.6
Well-Preserved 12 Kilometer Impact Crater on East Rim in Isidis Region: ESP_014016_1945 ESP_022376_1945 (Interval in Earth days: 652)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.52	98.4	-8.6	14.23	48.5	51.5
Comparative Gully Morphology: ESP_013934_1335 ESP_014000_1335 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.0	183.	6.35	-11.3	40.0	41.5
Dry Falls in the Southern Branch of Kasei Valles: ESP_013152_1980 ESP_013297_1980 (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
17.90	285.	3.51	15.70	60.2	58.1
A Fan in a Southern Highlands Crater: ESP_014159_1670 ESP_020106_1670 (Interval in Earth days: 464)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.7	157.	-7.0	7.119	34.6	56.0
Gullies Observed by MOC: ESP_012707_1445 ESP_013208_1445 (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
-35.4	201.	2.07	23.84	46.6	38.4
Martian Volcanic Vent with Elevated Rim: ESP_013008_1825 ESP_020801_1825 (Interval in Earth days: 607)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.452	259.	-3.3	21.93	52.7	53.7
Southeastern Asimov Crater: ESP_013334_1320 ESP_013967_1320 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-47.4	5.52	1.98	-15.8	41.6	42.4
Knobby Terrain in Sinus Meridiani Seen in MOC Image M03-01935: ESP_013756_1850 ESP_021905_1850 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.817	357.	0.67	27.44	45.2	49.2
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