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

Thermophysical Boundary West of Hebrus Valles: ESP_086345_2015 ESP_087123_2015 (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
21.09	124.	5.18	-9.06	39.9	43.0
A Slice through the Layercake: ESP_084979_1975 ESP_085045_1975 (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
17.49	336.	16.6	-4.34	44.6	45.3
Hillslope Morphologies in Crater: ESP_085793_1510 ESP_086294_1510 (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
-28.6	84.7	3.79	-4.91	47.1	55.3
Hillslope Morphologies near Holden Crater: ESP_085705_1550 ESP_085850_1550 (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
-24.7	325.	3.70	23.92	43.7	44.3
Small Delta or Fan: ESP_085751_1725 ESP_085962_1725 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-7.46	147.	8.32	-7.47	37.5	40.7
Kasei Valles Lava: ESP_085970_1965 ESP_086326_1965 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.39	285.	4.76	-6.69	38.9	40.3
Gullied Slope: ESP_085723_1370 ESP_085868_1370 (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
-42.8	197.	-4.7	10.24	55.4	56.9
Inverted Channel in Noachis Terra: ESP_085730_1505 ESP_085664_1505 (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
-29.2	5.09	-7.7	6.602	47.2	45.3
Possible Esker in Phlegra Montes: ESP_085948_2165 ESP_086673_2165 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.15	164.	-8.9	24.11	48.0	41.2
North Pole Facing Deposit in Crater: ESP_085774_2230 ESP_085853_2230 (Interval in Earth days: 7)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
42.65	234.	0.49	23.69	53.0	50.5
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