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

Small Crater in Amazonis Planitia: ESP_017361_1830 ESP_018073_1830 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.024	219.	-6.7	4.499	51.3	52.3
Polar Crater with Summer Ice: ESP_017510_2465 ESP_017945_2465 (Interval in Earth days: 34)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
66.39	99.7	-0.4	14.50	49.4	48.4
Layered Terrain in Aeolis and Zephyria Regions: ESP_017680_1775 ESP_018102_1775 (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
-2.31	149.	4.54	-12.8	54.6	56.5
Central Peak of an Impact Crater: ESP_017430_1910 ESP_018709_1910 (Interval in Earth days: 100)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.63	134.	-8.9	4.868	48.0	49.4
Possible Clay Beds in West Ladon Valles Channels: ESP_017489_1610 ESP_035119_1610 (Interval in Earth days: 1374)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.9	326.	-5.8	-19.4	65.4	66.3
Hellas Planitia Terrain: ESP_017644_1420 ESP_025925_1420 (Interval in Earth days: 645)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-37.8	56.7	5.17	-12.5	79.0	76.3
Central Uplift of an Impact Crater: ESP_017603_1550 ESP_026095_1550 (Interval in Earth days: 661)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.7	94.5	2.99	-24.4	69.4	68.6
Very Fresh Double Crater: ESP_017613_2195 ESP_017903_2195 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
39.31	174.	-11.	8.67	42.6	41.3
Tilted Block at Coprates Chasma and Debris Flows: ESP_017332_1680 ESP_018110_1680 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.8	291.	4.28	-8.27	59.3	62.0
Streamlined Landform with Benches in Kasei Valles System: ESP_017398_1970 ESP_017820_1970 (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
16.92	285.	9.39	-8.3	43.9	46.4
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