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

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
Lava Flow Oozing into a Crater: ESP_024587_1465 ESP_024877_1465 (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
-33.2	222.	7.47	28.63	55.5	58.7
Mawrth Vallis Stratigraphy Exposed: ESP_024200_2045 ESP_024055_2045 (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
24.47	341.	1.71	-15.1	39.2	41.2
Field of Transverse Aeolian Ridges in Proctor Crater: ESP_024449_1320 ESP_024515_1320 (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
-47.7	31.0	21.9	4.433	63.1	65.1
Gullies on the South Wall of Dao Vallis near the Confluence with Niger Vallis: ESP_024315_1435 ESP_031818_1435 (Interval in Earth days: 584)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.1	90.2	-5.0	8.408	53.9	35.4
Colorful Central Peak in an Unnamed Crater: ESP_023674_1590 ESP_024597_1595 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-20.5	306.	6.77	24.62	34.8	46.2
Rugged Banded Material in Crater in Northwest Hellas Planitia: ESP_023789_1420 ESP_024066_1420 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.7	47.4	21.8	0.082	44.7	50.6
Basal Exposure of South Polar Layered Deposits: ESP_023760_1065 ESP_032542_1065 (Interval in Earth days: 685)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-73.4	132.	-5.7	9.39	73.2	72.0
Libya Montes Layered Cliffs: ESP_023827_1835 ESP_024671_1835 (Interval in Earth days: 65)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.427	85.9	11.0	-9.63	32.7	38.9
Possible Exposures of Polar Layered Deposits in Area Not Well Observed: ESP_023793_0895 ESP_023673_0905 (Interval in Earth days: 9)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-89.2	49.1	24.5	24.15	86.2	83.8
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