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

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
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
Small Mounds in Chryse Planitia: ESP_024082_1995 ESP_023581_1995 (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
19.07	322.	7.16	-17.0	37.1	42.1
Cerberus Fossae Streak and Bedform Changes: ESP_024075_1930 ESP_024563_1930 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
12.74	154.	3.78	-23.4	35.2	38.4
Massif in Reull Vallis: ESP_024051_1365 ESP_024407_1365 (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
-43.2	97.0	7.01	22.35	53.8	59.0
Proctor Crater Dune Changes: ESP_024291_1320 ESP_024370_1320 (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
-47.6	30.3	-29.	-0.98	63.3	62.9
Harmakhis Vallis Terrain Sample: ESP_024249_1405 ESP_024394_1405 (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
-39.2	92.0	-1.1	16.31	54.7	56.2
Alluvial Fans and Hanging Valley Morphology in Kasei Valles: ESP_024215_2030 ESP_024637_2030 (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
22.69	291.	8.75	-2.72	37.8	37.9
Mantle Removal around Gully Fan: ESP_024027_1345 ESP_024304_1345 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.4	33.9	-5.9	-21.5	55.7	61.3
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