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

Clays and Chlorides in Sirenum Region: ESP_016043_1480 ESP_016188_1480 (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
-31.6	206.	-5.5	9.37	60.3	61.5
New Impact Site Formed Between January 2007 and May 2009: ESP_015949_1795 ESP_069449_1795 (Interval in Earth days: 4168)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.64	248.	-7.7	1.95	42.4	55.1
Non-Reticulate Bedforms: ESP_016068_1720 ESP_016213_1720 (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
-8.05	240.	-0.9	16.85	46.3	46.8
Bedrock Bench in Ganges Chasma: ESP_015907_1710 ESP_016830_1710 (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
-8.94	316.	-7.2	10.26	45.3	53.8
Gullied Slope of 20-Kilometer Diameter Impact Crater in Acidalia Planitia: ESP_016170_2230 ESP_016460_2230 (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
42.64	329.	0.01	21.35	44.4	41.3
Triple Ricochet Crater in Ascuris Planum: ESP_016185_2215 ESP_016462_2215 (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
41.30	279.	-0.0	-19.0	43.7	44.2
Central Peak of an Impact Crater in Terra Sabaea: ESP_016153_1565 ESP_020188_1565 (Interval in Earth days: 314)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.0	81.0	7.63	-4.44	55.4	59.1
Stratigraphic Relations in MOC Image M00-02426 in Sinus Meridiani: ESP_016169_1790 ESP_019637_1790 (Interval in Earth days: 270)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.77	1.73	4.18	-16.4	43.8	56.0
Layered Material Seen in MOC Image M0807392 in Focas Crater: ESP_016208_2135 ESP_017975_2135 (Interval in Earth days: 138)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
33.42	12.7	1.67	-15.9	41.0	43.8
Cratered Cones in Galaxias Colles: ESP_016269_2165 ESP_016348_2165 (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
36.30	147.	-0.3	26.74	41.8	39.2
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