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

Possible Chlorites and Prehnite in Northern Plains Crater: ESP_016933_2310 ESP_017210_2310 (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
50.48	16.5	4.76	-14.3	43.8	44.8
Fans in Unnamed Crater Southeast of Holden Crater: ESP_017278_1470 ESP_053725_1470 (Interval in Earth days: 2840)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-32.4	329.	-2.9	7.278	73.9	72.6
Strike Slip Faults in Amazonis Planitia: ESP_017045_2015 ESP_018113_2015 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
21.26	204.	-6.1	8.022	42.8	44.3
Thermally Distinct Crater in Arcadia Dorsa: ESP_017097_2340 ESP_017532_2340 (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
53.62	218.	3.64	24.24	44.5	42.0
Candidate MSL Landing Site in Northeast Syrtis Major: ESP_016931_1980 ESP_017076_1980 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.80	77.0	-4.2	8.612	43.0	42.6
Debris Apron Terrain in Deuteronilus Mensae: ESP_017170_2250 ESP_017671_2250 (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
44.66	28.3	-6.2	5.977	42.6	41.6
Nili Patera: ESP_016905_1890 ESP_035181_1890 (Interval in Earth days: 1424)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.910	67.6	0	17.66	45.7	47.4
Persbo Crater Ejecta Covered by Lava Flows: ESP_017060_1890 ESP_017205_1890 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.912	156.	-8.7	5.039	47.2	46.8
Light-Toned Mounds in Acidalia Planitia: ESP_017132_2250 ESP_017633_2250 (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
44.43	345.	-6.6	5.659	42.7	41.6
Possible Intact Layers in Crater Central Uplift: ESP_017055_1975 ESP_017833_1975 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.36	291.	-0.5	-13.7	43.4	46.7
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