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

Streamlined Landforms adjacent to Shalbatana Vallis: ESP_080299_1895 ESP_080444_1895 (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
9.172	318.	-13.	12.02	54.3	52.6
Traverse Ramp in East Coprates Chasma: ESP_080405_1640 ESP_079983_1640 (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
-15.8	307.	-4.1	-14.2	66.2	67.4
Grooves and Cataracts in Eos Chasma: ESP_080576_1665 ESP_080431_1665 (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
-13.3	318.	-0.6	-16.6	64.1	65.6
Curvilinear Ridges on Floor of Shalbatana Vallis: ESP_080589_1885 ESP_080233_1885 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.367	318.	19.4	-1.16	52.6	53.6
Juventae Chasma Interior Deposit Layers: ESP_080458_1755 ESP_080669_1755 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.62	297.	11.5	-0.14	58.9	59.5
Possible Dipping Layers in Ice-Affected Crater: ESP_080515_2115 ESP_080805_2115 (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
31.38	178.	-3.2	15.42	49.2	49.7
Possible Gully-Glacial Interaction in Utopia Planitia: ESP_080293_2195 ESP_080425_2195 (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
39.10	116.	5.5	-20.1	46.9	50.1
Streamlined Features in Athabasca Valles: ESP_080595_1890 ESP_080740_1890 (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
8.663	156.	6.28	17.47	53.5	52.9
Dunes near Syrtis Major Planum Crater Ejecta: ESP_080242_1970 ESP_080308_1970 (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
16.58	72.6	-8.3	-24.6	51.1	52.7
Light-Toned Exposures in Margaritifer Terra: ESP_080417_1750 ESP_079296_1750 (Interval in Earth days: 87)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.13	339.	-20.	-8.88	61.4	59.2
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