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

Channel Edge with Overbank Flow Deposits: ESP_083033_1835 ESP_082967_1835 (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
3.456	195.	7.43	29.20	57.0	55.5
Buried Crater on Ice-Rich Plateau on Malea Patera: ESP_083065_1170 ESP_083289_1170 (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
-62.9	53.3	-2.6	23.60	57.6	52.6
Ancient Crust Outcrops at Nectaris Montes: ESP_082950_1650 ESP_082884_1650 (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
-14.7	304.	2.16	26.28	52.4	51.0
Scour Pit Island in Southeastern Part of Medusae Fossae Formation: ESP_083046_1795 ESP_083191_1795 (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
-0.69	201.	-0.6	13.40	55.9	53.9
Crater with Steep Slopes: ESP_083268_1375 ESP_083624_1375 (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
-42.0	266.	-6.4	2.905	48.4	43.1
Streamlined Features in Argyre Planitia: ESP_083108_1320 ESP_083042_1320 (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
-47.5	316.	-9.5	8.121	52.2	51.9
Juventae Chasma Interior Deposit Layers: ESP_082937_1760 ESP_082357_1760 (Interval in Earth days: 45)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.16	297.	8.05	-7.44	54.7	58.4
Inverted Fluvial Channel or Channel Belt: ESP_083040_1990 ESP_083462_1990 (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
18.88	0.46	28.0	21.93	62.9	62.1
Athabasca Valles: ESP_083074_1895 ESP_083140_1895 (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
9.230	156.	-4.3	-26.0	60.3	61.7
Hillslope Morphologies near Holden Crater: ESP_083002_1550 ESP_083859_1550 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.8	325.	7.31	20.89	50.2	38.3
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