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

Crater with Channel : ESP_046123_1790 ESP_055129_1790 (Interval in Earth days: 702)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.88	158.	-3.1	-28.7	51.1	54.8
Western Half of Rayed Pebas Crater : ESP_045997_1775 ESP_046142_1775 (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
-2.61	-0.9	-6.3	8.161	51.8	50.7
Louth Crater Ice Mound : ESP_045887_2505 ESP_045439_2505 (Interval in Earth days: 35)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
70.22	103.	18.0	-8.26	62.4	58.1
Small Tributary Deposit and Transverse Aeolian Ridges in Nirgal Vallis : ESP_045814_1520 ESP_046592_1520 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.6	317.	5.48	-4.70	63.3	57.8
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
Potential Fluid Flow on Top of Ejecta Layer : ESP_046086_2140 ESP_046231_2140 (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
33.60	84.4	-5.4	5.999	51.1	52.0
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
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
Syria Planum Bedform and Albedo Changes : ESP_046080_1655 ESP_046502_1655 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.2	252.	22.2	7.064	53.8	53.2
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