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

Layer and Color Boundaries at Mawrth Vallis: ESP_033615_2030 ESP_033905_2030 (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
22.51	342.	-0.4	27.14	38.7	36.8
Enigmatic Channel Carved into the Floor of Mangala Valles: ESP_033686_1635 ESP_033831_1635 (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
-16.1	210.	-23.	-7.27	51.4	52.2
Possible Smectite Deposits in Northwest Hellas Region: ESP_033652_1580 ESP_041907_1580 (Interval in Earth days: 643)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-21.6	57.2	2.99	20.83	52.5	43.8
Light-Toned Layered Deposits Exposed along Ladon Valles Floor: ESP_033642_1585 ESP_033787_1585 (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
-21.0	330.	-3.9	12.32	52.4	53.4
Pit South of Arsia Mons: ESP_033342_1660 ESP_050089_1660 (Interval in Earth days: 1305)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.8	240.	-0.3	-8.91	43.9	32.6
High-Lava Mark in Kasei Valles: ESP_033617_1990 ESP_034316_1990 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.64	285.	20.6	-9.79	36.5	42.1
Gullies in Central Peak of Hale Crater: ESP_033695_1445 ESP_024346_1445 (Interval in Earth days: 729)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.3	323.	18.6	-1.51	61.4	53.6
Eastern Rim of Well-Preserved Crater on Northern Plains: ESP_033684_2355 ESP_033974_2355 (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
55.34	253.	-5.1	12.28	51.7	48.1
Lava-Embayed Crater in Kasei Valles: ESP_033590_2055 ESP_034078_2055 (Interval in Earth days: 38)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.39	301.	26.4	0.83	36.7	39.6
Pit or Crater near Galaxias Chaos: ESP_033332_2155 ESP_042088_2155 (Interval in Earth days: 683)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
35.10	146.	0.31	28.38	43.1	41.8
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