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

Monitor Opposing Barchan Dunes and Star Dunes : ESP_059292_1310 ESP_058646_1310 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-48.4	282.	14.4	-8.91	56.3	46.8
Lava Flows Embaying Impact Crater: ESP_059452_1540 ESP_076135_1540 (Interval in Earth days: 1300)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.9	232.	-0.5	-15.5	44.0	37.4
Gullied Lobate Flow Features : ESP_059436_1335 ESP_059001_1335 (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
-46.3	310.	14.6	-19.1	57.1	51.5
Impact Crater with Central Pit : ESP_059263_1840 ESP_059408_1840 (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
4.060	349.	-8.6	7.628	33.4	32.6
Mounds in Chryse Planitia : ESP_058974_2245 ESP_059475_2245 (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
44.03	313.	-3.7	11.54	56.2	49.1
Glacier Moving Upslope Near Reull Vallis : ESP_058916_1370 ESP_059338_1370 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-42.7	108.	4.53	-8.97	46.2	54.0
Western Half of Well-Preserved Impact Crater : ESP_058921_2020 ESP_059422_2020 (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
21.61	324.	-6.8	13.21	41.1	36.3
Scamander Vallis : ESP_058800_1965 ESP_058589_1965 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.03	28.4	-4.5	7.472	38.7	40.1
Smooth Region in Phlegra Montes : ESP_058729_2170 ESP_059006_2170 (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
36.54	162.	7.97	-17.3	53.1	50.9
Gullies in Crater in Terra Cimmeria : ESP_058901_1335 ESP_067341_1335 (Interval in Earth days: 657)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.9	158.	1.39	29.38	48.4	45.6
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