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

Chaos Terrain in Small Impact Crater : ESP_058965_1495 ESP_059255_1495 (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
-30.3	210.	-20.	5.926	40.6	43.2
Slope Monitoring : ESP_058715_1500 ESP_059348_1500 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-29.5	194.	4.51	-20.7	35.1	45.9
Polyphase Exit Breach in Small Crater on East Rim of Holden Crater : ESP_058987_1545 ESP_059053_1545 (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
-25.4	327.	4.33	-17.8	36.5	38.9
Gullies from Layers in Asimov Crater in MOC Image R1600339 : ESP_058788_1320 ESP_067703_1320 (Interval in Earth days: 694)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-47.5	4.65	-4.2	8.752	48.1	53.5
Possible Exit Breaches in Crater with Preserved Ejecta Texture : ESP_058921_1575 ESP_058710_1575 (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
-22.3	328.	5.09	15.81	34.2	31.2
Crater Breach and Kasei Valles Lava Flow : ESP_058830_2040 ESP_058540_2040 (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
23.79	287.	7.29	-13.5	42.5	47.1
Potential Landing Site in Phlegra Montes : ESP_058874_2160 ESP_059296_2160 (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
35.84	164.	8.55	-4.42	50.6	46.4
Scalloped Depressions in Amphitrites Patera : ESP_058997_1220 ESP_058931_1220 (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
-57.6	61.2	-8.2	5.8	59.5	57.7
Well-Preserved Alluvial Fans in Complex Crater within Isidis Planitia : ESP_058969_1905 ESP_059391_1905 (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
10.45	94.3	2.65	-12.5	34.3	34.9
Layered Deposits from Crater Floor to Rim : ESP_058788_1890 ESP_066542_1890 (Interval in Earth days: 604)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.746	358.	-17.	-8.20	36.0	52.0
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