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

Isolated Layered Mound in Trough Between Layered Benches in Terby Crater: ESP_016628_1520 ESP_016773_1520 (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
-27.6	74.4	0.18	16.62	64.9	65.4
Submerged Rim of Crater and Floor Deposits from Uzboi Vallis: ESP_016487_1495 ESP_017120_1495 (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
-30.0	323.	11.7	-6.42	64.1	71.3
Lobate Tongue Terminus in CTX Image: ESP_016418_2255 ESP_017130_2255 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
45.06	38.1	-2.1	10.57	44.3	41.3
Crater West of Niesten Crater: ESP_016510_1515 ESP_019279_1515 (Interval in Earth days: 216)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.2	56.2	-2.9	14.98	64.0	66.9
Small Volcano in Tharsis Region: ESP_016806_2005 ESP_016872_2005 (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
20.15	247.	16.4	-3.58	40.3	42.2
Ejecta of Crater Sectioned by Erosion: ESP_016896_1710 ESP_025678_1710 (Interval in Earth days: 684)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.92	315.	6.04	-5.75	54.6	53.8
Interesting Crater Ejecta in Columbus Crater: ESP_016861_1505 ESP_017639_1505 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-29.3	193.	1.16	-12.7	68.3	73.7
Wrinkle Ridges in Hesperia Planum: ESP_016455_1535 ESP_016811_1535 (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
-26.2	117.	-5.9	7.118	62.1	65.3
Deposit Associated with Channels along Floor of Ganges Chasma: ESP_016817_1710 ESP_017239_1710 (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
-8.69	311.	5.05	-13.5	53.8	57.9
Possible Phyllosilicates: ESP_016891_1710 ESP_017669_1710 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.92	91.9	2.12	-13.6	54.8	59.8
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