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

Ostrov Crater Fans and Playa: ESP_017357_1530 ESP_026561_1530 (Interval in Earth days: 718)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.5	331.	-6.1	-18.2	70.2	71.3
Layered Terrain in Aeolis and Zephyria Regions: ESP_017680_1775 ESP_018102_1775 (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
-2.31	149.	4.54	-12.8	54.6	56.5
Central Uplift of an Impact Crater: ESP_017434_1525 ESP_027139_1525 (Interval in Earth days: 757)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.0	29.6	-4.8	16.90	70.8	69.6
Central Peak of Vivero Crater: ESP_017338_2295 ESP_017760_2295 (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
48.97	118.	7.86	-3.18	42.2	43.3
Western Half of Fresh Crater on Alba Patera: ESP_017571_2235 ESP_017861_2235 (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
43.05	240.	-9.5	10.32	42.5	41.3
Fresh Impact Crater in MOC M23-01705: ESP_017490_2315 ESP_018901_2315 (Interval in Earth days: 110)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
51.25	289.	0.1	-18.3	43.4	51.5
Valley along Noctis Labrynthus Floor: ESP_017465_1730 ESP_017966_1730 (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
-7.16	261.	-10.	10.24	57.8	57.8
Well-Preserved 1-Kilometer Diameter Impact Crater on Northern Plains: ESP_017480_2355 ESP_017968_2355 (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
55.21	200.	6.86	-14.0	44.1	46.3
Laminar Flow in Ejecta Layer North of Tooting Crater: ESP_017625_2040 ESP_018258_2040 (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
23.80	207.	2.38	-18.9	42.9	46.3
Viscous Flows and Persbo Crater Ejecta East of Athabasca Valles: ESP_017350_1890 ESP_017772_1890 (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
8.749	157.	8.43	-10.0	47.2	49.9
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