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

Scarps in Utopia Planitia : ESP_045808_2090 ESP_046309_2090 (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
28.74	114.	0	14.75	46.7	51.0
Clustered Mounds with Trough-Shaped Depressions : ESP_045820_1920 ESP_055472_1920 (Interval in Earth days: 752)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.75	149.	1.09	19.64	47.3	51.6
Fractures in Utopia Planitia : ESP_046151_2140 ESP_046573_2140 (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
33.84	108.	4.82	-6.29	51.2	57.7
Streamlined Shape in Marte Vallis : ESP_045911_1995 ESP_046412_1995 (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
19.27	184.	-4.7	13.68	47.6	50.2
Pits and Lava in Amazonis Planitia : ESP_045818_1965 ESP_046240_1965 (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
16.13	202.	5.08	-13.5	46.3	50.8
Ridges in Cydonia Region : ESP_045918_2160 ESP_046419_2160 (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
35.61	351.	-5.8	9.679	49.6	55.0
Crater with Blocky Interior in Marte Vallis : ESP_045977_1920 ESP_046267_1920 (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
11.83	183.	-6.5	20.42	48.6	48.0
Candidate Landing Site for 2020 Mission in Jezero Crater : ESP_045994_1985 ESP_046060_1985 (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
18.42	77.4	3.48	-18.2	47.5	49.9
1-Kilometer Diameter Crater : ESP_046065_2260 ESP_046355_2260 (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
45.84	295.	-5.3	13.65	54.8	57.7
East Coprates Montes Dark Fans : ESP_045907_1665 ESP_046619_1665 (Interval in Earth days: 56)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.3	297.	-2.1	12.58	55.8	52.1
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