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

Proposed Site for Future Exploration at Ladon Valles: ESP_024438_1595 ESP_024860_1595 (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
-20.1	329.	0.98	-22.2	45.2	52.8
Bedform and Sand Changes in Southwestern Utopia Planitia: ESP_024499_2110 ESP_024433_2110 (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
30.71	97.7	1.24	20.88	40.5	39.3
Meanders and Tributaries in Ridge Form in the Zephyria Region: ESP_024484_1750 ESP_024985_1750 (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
-5.09	151.	4.43	19.16	38.5	43.0
Dune Composition: ESP_025042_1375 ESP_024976_1375 (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
-42.3	42.0	0.35	18.39	69.4	67.5
Lava Coating, Flood-Carved Kasei Valles: ESP_024202_2010 ESP_024703_2010 (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
20.84	287.	-2.9	19.15	38.0	35.7
The Eastern Floor of Aram Chaos: ESP_024266_1830 ESP_023910_1830 (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
3.112	340.	24.6	9.188	33.0	32.9
Landforms Including Fans in Terrain Northwest of Gale Crater: ESP_023944_1775 ESP_026990_1775 (Interval in Earth days: 237)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.56	135.	-24.	1.169	35.7	54.8
Windstreak and Bedform Changes: ESP_024241_1985 ESP_025085_1985 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.24	302.	-0.0	-28.1	36.9	41.0
Well-Preserved 8 Kilometer Crater: ESP_024080_1340 ESP_032928_1340 (Interval in Earth days: 690)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.4	25.7	6.66	20.83	55.9	56.0
Prominent Channel Form on Tyrrhena Patera: ESP_024222_1590 ESP_024723_1590 (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
-20.9	107.	-7.9	15.92	43.1	48.9
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