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

Terrain Northwest of Hellas Planitia: ESP_019543_1465 ESP_019899_1465 (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
-33.1	50.7	0	11.96	68.5	64.4
Mass Movement on Wall of Crater in Lyot Crater Ejecta Blanket: ESP_019438_2340 ESP_027231_2340 (Interval in Earth days: 607)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
53.55	26.3	-5.5	13.83	57.7	44.7
Fissures in Tempe Terra: ESP_019508_2245 ESP_019574_2245 (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
43.91	276.	-3.8	-18.2	55.2	57.3
Ismenius Cavus: ESP_019333_2140 ESP_019478_2140 (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
33.77	16.9	-14.	-2.15	51.9	52.3
Western Half of Crater in Sinus Sabaeus: ESP_019307_1715 ESP_019808_1715 (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
-8.50	12.3	-21.	6.908	59.3	56.0
Barchan Dunes in Dulovo Crater Region: ESP_019357_1835 ESP_027216_1835 (Interval in Earth days: 613)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
3.672	84.6	-7.6	7.029	53.8	51.2
Western End of Athabasca Valles Lava: ESP_019566_1855 ESP_025513_1855 (Interval in Earth days: 463)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
5.276	137.	0	-8.47	53.2	45.2
Monitoring of Pits and Fractures in Deuteronilus Mensae: ESP_019504_2240 ESP_019570_2240 (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
43.81	25.2	1.42	-13.1	54.7	56.8
Wavy Stratification Features in Crater Wall in MOC Image S14-00005: ESP_019558_1800 ESP_020125_1800 (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
0.165	357.	-10.	0.304	55.2	54.8
Claritas Fossae Region with Possible Serpentine: ESP_019509_1530 ESP_019654_1530 (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
-26.8	258.	-8.0	9.024	66.0	63.8
	Page 641 of 878 (8,772 images)