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

Gullied Trough Wall: ESP_012602_1415 ESP_013881_1415 (Interval in Earth days: 100)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-38.3	188.	6.27	18.92	48.1	35.6
Northwest Wall of Juventae Chasma: ESP_013244_1760 ESP_030228_1760 (Interval in Earth days: 1323)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.14	296.	0	10.99	46.6	50.0
Pit on Crater Floor Exposing Layers: ESP_012818_1560 ESP_013174_1560 (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
-23.8	50.3	-6.3	4.629	46.1	40.7
High-Latitude Gullies: ESP_013453_1075 ESP_022789_1075 (Interval in Earth days: 728)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-72.2	3.84	0.52	-16.3	54.5	58.2
Differential Erosion of Light-Toned Stratigraphy in Melas Chasma: ESP_013640_1710 ESP_012928_1710 (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
-8.93	285.	8.51	-10.3	39.1	48.9
Ridges at the Edge of the Layered Deposits within Reynolds Crater: ESP_013169_1055 ESP_013301_1055 (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
-74.2	200.	-3.6	-17.2	56.4	57.0
Gullies: ESP_012734_1265 ESP_012879_1265 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-53.1	188.	-7.8	2.791	50.7	47.9
Basal Exposure of South Polar Layered Deposits: ESP_013290_1075 ESP_013092_1075 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-72.2	138.	-18.	5.428	55.8	55.0
Central Uplift of an Impact Crater in Hesperia Planum: ESP_013211_1675 ESP_013633_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
-12.4	118.	8.88	-5.92	42.9	39.0
Layers in Spallanzani Crater: ESP_013041_1215 ESP_013120_1215 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-58.1	86.8	5.04	26.10	48.1	45.8
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