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

Sinuous Ridge in Tempe Terra: ESP_062048_2240 ESP_061969_2240 (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
43.79	275.	3.55	-23.9	41.3	43.6
Crater in Utopia Planitia: ESP_062108_2210 ESP_069732_2210 (Interval in Earth days: 594)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.57	78.6	-2.3	11.41	41.7	47.3
Ice-Filled Impact: ESP_061885_2615 ESP_061911_2615 (Interval in Earth days: 2)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
81.33	32.5	-8.5	6.909	57.8	57.0
Layering in the Medusae Fossae Formation: ESP_061921_1770 ESP_063279_1770 (Interval in Earth days: 106)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.95	149.	-2.9	13.08	54.8	55.1
Crater in Arabia Terra: ESP_062137_2140 ESP_061781_2140 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
33.62	5.22	21.4	6.959	39.8	40.0
Leveed Rugged Lava Flow in Daedalia Planum: ESP_061931_1555 ESP_062076_1555 (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
-24.2	238.	6.92	27.38	68.4	67.4
Crater in Arabia Terra: ESP_061583_2245 ESP_061728_2245 (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
44.04	10.1	-7.7	7.48	41.4	40.3
Well-Preserved Impact Crater in Phlegra Montes: ESP_061617_2155 ESP_063331_2155 (Interval in Earth days: 134)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.92	162.	-4.2	23.65	40.5	48.3
Crater in Arabia Terra: ESP_061636_2130 ESP_061570_2130 (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
32.50	5.11	-8.7	6.895	41.1	39.6
Spectrally Distinct Crater Ejecta in Tyrrhena Terra : ESP_061686_1725 ESP_061620_1725 (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
-7.66	84.6	-2.9	17.22	57.0	55.5
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