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

Fan in Crater North of Nepenthes Mensae: ESP_088705_1815 ESP_088916_1815 (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
1.468	133.	4.91	-7.86	54.8	55.9
Lobate Glacial Deposit in Crater: ESP_088601_2150 ESP_088825_2150 (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
34.85	90.4	-8.8	26.07	44.8	42.4
Monitoring Gullied Crater: ESP_088568_2310 ESP_088634_2310 (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
50.71	266.	8.41	-6.17	44.4	45.9
Structure of Viscous Flow Feature Exposed by Ice Degradation: ESP_088510_2220 ESP_088431_2220 (Interval in Earth days: 7)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.58	51.9	11.0	-13.2	42.7	44.7
Kasei Valles Alluvial Fans: ESP_088633_2040 ESP_088778_2040 (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
23.55	298	-6.4	3.817	46.5	46.1
Channels along Hydraotes Chaos Channel: ESP_088566_1835 ESP_088711_1835 (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
3.377	329.	3.41	14.35	53.8	53.2
Jezero Crater: ESP_088707_1985 ESP_088773_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
18.47	77.5	0.57	-21.6	47.7	49.7
Stunning Outcrop in Nilosyrtis Mensae: ESP_088681_2160 ESP_088892_2160 (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
35.47	65.6	-5.2	-14.7	44.7	46.4
Pitted Cones in Aurorae Chaos: ESP_088540_1720 ESP_089107_1720 (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
-7.77	320.	3.86	-8.75	60.1	60.9
Fan-Shaped Feature in Ismenius Lacus: ESP_088485_2145 ESP_088696_2145 (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
33.95	17.5	-4.9	-15.7	44.2	45.9
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