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

Collapse Features on Hrad Vallis Mudflow: ESP_016467_2155 ESP_016533_2155 (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
35.13	141.	0.42	-15.9	41.1	42.4
Source Region for Branch of Auqakuh Vallis: ESP_016826_2080 ESP_016971_2080 (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
27.47	62.7	-7.7	5.246	41.4	40.6
Wrinkle Ridges in Hesperia Planum: ESP_016455_1535 ESP_016811_1535 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.2	117.	-5.9	7.118	62.1	65.3
Small Volcano in Northern Syria Planum: ESP_016318_1710 ESP_016951_1710 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.76	254.	6.70	-9.92	48.9	55.9
Light-Toned Layering in Hebes Mensa: ESP_016462_1785 ESP_016818_1785 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.35	282.	0.48	14.17	47.0	49.0
Ejecta Flow and Obstacle at Arandas Crater: ESP_016776_2225 ESP_016842_2225 (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
42.39	344.	4.98	-9.79	41.8	43.0
Large-Scale Slumping in Moreux Crater: ESP_016642_2215 ESP_017710_2215 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
41.13	44.1	-7.3	6.121	42.8	41.2
Northern Plains West of Erebus Montes: ESP_016650_2205 ESP_035427_2205 (Interval in Earth days: 1464)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.26	185.	-1.2	27.98	42.1	39.3
Floor of Cut Crater: ESP_016461_1680 ESP_025533_1680 (Interval in Earth days: 707)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-11.8	312.	-6.7	15.71	53.1	53.0
Potential Rhythmic Layering in East Gale Crater with Hydrated Signature: ESP_016375_1750 ESP_016520_1750 (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
-5.15	138.	1.01	18.09	48.0	48.2
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