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

Possible Phyllosilicates: ESP_016891_1710 ESP_017669_1710 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-8.92	91.9	2.12	-13.6	54.8	59.8
Fresh Crater on Alba Patera: ESP_016371_2235 ESP_016226_2235 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
43.05	240.	4.58	-7.09	43.2	44.8
Eroded Material Adjacent to Cerberus Fossae: ESP_016506_1890 ESP_017495_1890 (Interval in Earth days: 77)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.114	160.	2.89	-11.8	42.9	49.1
Aram Chaos Mineralogical Variability: ESP_016605_1830 ESP_086812_1830 (Interval in Earth days: 5470)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.889	339.	-8.3	-23.3	46.9	47.0
Possible Landslide Triggered by Impact: ESP_016386_1475 ESP_016531_1475 (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
-32.4	201.	1.20	16.67	65.1	65.9
Crater Superposed on Mamers Vallis Seen in MOC Image R1802279: ESP_016366_2125 ESP_016511_2125 (Interval in Earth days: 12)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
31.95	18.7	8.24	20.96	40.0	38.7
Degradation of Old Crater Rim on Northwest Slope of Acheron Fossae: ESP_016873_2185 ESP_017018_2185 (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
38.30	218.	-8.3	1.584	42.0	41.0
Crater with Central Uplift Northwest of Argyre Planitia: ESP_016712_1435 ESP_018914_1435 (Interval in Earth days: 172)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-36.1	302.	-0.8	14.26	71.9	74.4
Terrain South of Newcomb Crater: ESP_016736_1520 ESP_068970_1525 (Interval in Earth days: 4070)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.6	5.59	4.65	-7.50	65.7	63.9
Extensive Crater Ejecta Blanket in Galaxias Colles: ESP_016704_2180 ESP_017337_2180 (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
37.86	150.	8.31	-9.63	40.7	42.0
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