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

Pavonis Mons Caldera Wall: ESP_078561_1810 ESP_078851_1810 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
0.816	246.	-29.	-0.86	53.4	53.2
Terrain in Xanthe Dorsa: ESP_078307_2205 ESP_079164_2205 (Interval in Earth days: 66)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.40	334.	-4.5	14.17	44.2	42.2
Scarp in Claritas Fossae: ESP_078218_1575 ESP_078152_1575 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-22.4	254.	-26.	-3.06	63.2	61.0
Northern Mid-Latitude Terrain: ESP_078339_2115 ESP_087200_2115 (Interval in Earth days: 690)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
31.13	181.	3.47	-7.62	42.2	42.6
Ice Flow Features between Craters: ESP_078247_2185 ESP_078313_2185 (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
38.25	172.	3.75	-13.7	43.1	44.5
Crater Rim: ESP_078506_2130 ESP_088501_2130 (Interval in Earth days: 779)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
32.66	301.	2.76	-13.4	42.5	45.1
Tributary Flowing through Crater Rim nearby Aram Chaos: ESP_078452_1870 ESP_079441_1870 (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
6.909	339.	5.16	-5.9	47.3	52.9
Crater-Edge Mounds in Chryse Planitia: ESP_078584_2055 ESP_078729_2055 (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
25.36	333.	-5.1	7.302	43.7	43.0
Faulted Alluvial Fan and Catchment in Eos Chasma: ESP_078321_1660 ESP_086338_1660 (Interval in Earth days: 624)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.6	318.	3.24	25.26	56.9	45.2
Alluvial Fans in Kasei Valles: ESP_077966_1980 ESP_078032_1980 (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
17.91	285.	25.5	3.616	39.6	41.9
	Page 108 of 881 (8,805 images)