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

Lineated Valley Fill Near Deuteronilus Region: ESP_016168_2180 ESP_024594_2180 (Interval in Earth days: 656)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.78	23.8	4.56	-7.15	42.2	43.8
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 Crater: ESP_016263_2310 ESP_016553_2310 (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
50.59	308.	3.22	21.47	47.2	43.9
Sulfate Layered Stratigraphy in Ophir Region: ESP_015974_1760 ESP_020220_1760 (Interval in Earth days: 331)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-3.85	285.	4.82	-15.3	43.0	56.3
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
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
Large Polygons: ESP_016098_1415 ESP_016164_1415 (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
-38.1	144.	7.55	-11.8	64.9	66.9
Well-Preserved 3-Kilometer Diameter Gullied Crater: ESP_016002_2285 ESP_016134_2285 (Interval in Earth days: 10)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
47.99	234.	1.86	-24.6	47.8	49.0
Possible MSL Landing Site in Mawrth Vallis: ESP_015985_2040 ESP_016262_2040 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.82	341.	13.7	-11.8	38.3	40.8
Layer Exposure in Crater North of Meridiani Planum: ESP_015958_1835 ESP_016235_1835 (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
3.571	1.15	11.6	-17.7	39.8	44.4
	Page 706 of 885 (8,850 images)