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

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
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
Well-Preserved Impact Crater: ESP_012851_1270 ESP_013695_1270 (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
-52.8	234.	-10.	-26.8	49.2	45.2
Wrinkle Ridge in Hesperia Planum: ESP_013765_1605 ESP_014187_1605 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-19.3	114.	2.67	-13.1	35.4	34.5
Lobate Features in the Charitum Montes: ESP_013165_1275 ESP_013244_1275 (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
-51.9	301.	-4.0	20.40	45.0	42.6
Gullies Observed by MOC: ESP_012707_1445 ESP_013208_1445 (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
-35.4	201.	2.07	23.84	46.6	38.4
Sulfate Beds in Gale Crater with Possible Repeating Section: ESP_012907_1745 ESP_013540_1745 (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
-5.32	137.	5.49	-16.2	49.5	43.6
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
Superb Phyllosilicate Mafic Stratigraphy Northwest of Hellas Planitia: ESP_012923_1540 ESP_013345_1540 (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
-25.9	63.8	-4.0	-17.6	44.3	40.2
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