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

Dune Monitoring in Northern Mid-Latitude Crater: ESP_088230_2400 ESP_088454_2400 (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
59.81	135.	-4.2	14.96	47.5	46.2
Flow in Tharsis Region: ESP_088055_2035 ESP_088345_2035 (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
23.45	241.	-21.	-5.64	46.3	45.7
Canyon Wall and Floor in Coprates Chasma: ESP_088290_1655 ESP_088501_1655 (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
-14.2	306.	8.94	-6.79	63.5	64.9
Bench in Mangala Valles: ESP_088109_1710 ESP_088676_1710 (Interval in Earth days: 44)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.95	208.	5.01	-16.7	59.8	62.3
Pedestal Crater Marginal Pits: ESP_088126_2400 ESP_088205_2400 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
59.79	96.3	-9.1	6.586	47.8	46.5
Dune Monitoring in North Mid-Latitude Crater: ESP_088311_2350 ESP_088377_2350 (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
54.61	83.4	5.81	-7.40	45.0	46.2
Jezero Crater: ESP_088061_1985 ESP_088272_1985 (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
18.47	77.3	-10.	-24.7	46.9	48.7
Dune Field: ESP_088035_2385 ESP_088378_2385 (Interval in Earth days: 26)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
57.96	58.8	6.11	-24.3	45.9	48.8
Channel South of Janssen Crater: ESP_088168_1800 ESP_088458_1800 (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
0.118	37.6	-7.2	12.15	55.4	54.8
Kasei Valles Scarps and Terraces: ESP_088145_2055 ESP_088567_2055 (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
25.39	302.	-3.6	-28.6	44.6	48.0
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