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

Faulting in South Polar Layered Deposits: ESP_012762_1070 ESP_013171_1070 (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
-72.9	146.	10.3	-12.8	58.0	56.3
Rayed Crater: ESP_013955_1020 ESP_013968_1020 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-77.8	345.	-6.7	7.228	62.3	61.6
Putative Paleolake: ESP_013780_1630 ESP_058667_1630 (Interval in Earth days: 3497)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-16.7	64.7	1.57	-15.2	35.8	31.8
Cratered Cones in Galaxias Colles: ESP_012946_2165 ESP_013236_2165 (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
36.17	147.	4.76	26.24	74.0	71.2
Crater Gully Morphology: ESP_013670_1435 ESP_013815_1435 (Interval in Earth days: 11)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.2	190.	3.34	14.46	36.5	35.3
Western Slope of Asimov Crater: ESP_013110_1325 ESP_013611_1325 (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
-47.0	4.17	-23.	-7.91	45.4	41.0
Marte Vallis Streamlined Landforms: ESP_014092_1955 ESP_014158_1955 (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
15.46	183.	-6.8	-25.9	48.1	48.6
Central Structure of a Large Impact Crater: ESP_013134_1610 ESP_021494_1610 (Interval in Earth days: 652)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.6	62.6	-6.3	14.94	43.1	44.9
Possible Clay and Sulfate in Terra Sirenum Layered Deposit: ESP_013485_1535 ESP_013907_1535 (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
-26.0	199.	4.43	-12.0	36.9	35.3
Light-Toned Material in a Crater in Iani Chaos: ESP_013572_1795 ESP_022710_1795 (Interval in Earth days: 712)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.54	341.	-3.2	13.82	44.7	37.9
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