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

Concentric Crater Fill: ESP_090042_2190 ESP_089686_2190 (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
38.47	347.	2.90	-10.3	54.9	52.0
Light-Toned Exposures in Capri Chasma: ESP_090215_1670 ESP_090149_1670 (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
-12.9	312.	-3.4	16.26	60.6	59.3
Light-Toned Exposures in Capri Chasma: ESP_090004_1670 ESP_089938_1670 (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
-13.0	312.	-5.2	15.64	61.4	60.1
Dune Interaction with Residual Polar Ice: ESP_089932_2600 ESP_090156_2600 (Interval in Earth days: 18)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
79.66	99.1	-7.9	1.407	70.2	73.1
Landing Site Characterization for Possible Future Rotorcraft : ESP_090127_2185 ESP_089204_2185 (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
38.18	186.	4.89	-13.2	55.7	48.1
Dune Monitoring in Nilosyrtis Mensae: ESP_090092_2110 ESP_089947_2110 (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
30.73	63.1	7.05	-9.93	53.7	53.7
Possible Skylight Showing Thermal Anomaly in Young Lava Flows: ESP_089930_1890 ESP_090286_1890 (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
8.718	169.	-5.8	16.74	54.6	54.1
Impact Crater Exposing Structure within Lobate Debris Apron: ESP_090278_2205 ESP_089988_2205 (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
39.92	23.0	18.4	-11.9	56.9	55.8
Lava Falls in Kasei Valles: ESP_089952_2025 ESP_090097_2025 (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
22.09	286.	7.26	24.46	52.0	51.6
Planned ExoMars Landing Site in Oxia Planum: ESP_089726_1975 ESP_089225_1975 (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
17.14	336.	11.0	-14.0	50.8	50.8
	Page 1 of 873 (8,723 images)