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

Cones in Acidalia Region: ESP_014258_2210 ESP_022974_2210 (Interval in Earth days: 679)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.53	326.	6.91	26.01	63.5	63.2
Gullies and Pasted on Material in Nereidum Montes: ESP_014391_1365 ESP_050192_1365 (Interval in Earth days: 2790)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-43.2	310.	-23.	8.653	44.2	47.8
Western Edge of Layered Mound in Juventae Chasma: ESP_014378_1755 ESP_020470_1755 (Interval in Earth days: 475)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.47	297.	-4.8	16.67	35.3	53.4
Tractus Catena: ESP_014432_2110 ESP_023135_2110 (Interval in Earth days: 678)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
30.77	257.	5.46	-19.5	53.6	55.4
Very Fresh 1-Kilometer Diameter Impact Crater: ESP_014405_1635 ESP_021776_1635 (Interval in Earth days: 575)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-16.2	281.	-5.4	26.42	33.9	41.2
Multiple Branches of the Cerberus Fossae: ESP_014383_1910 ESP_022097_1910 (Interval in Earth days: 601)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.66	158.	0.24	-14.4	41.3	53.7
Well-Preserved 7-Kilometer Diameter Gullied Crater in Newton Region: ESP_014395_1425 ESP_022188_1425 (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
-37.2	198.	-8.2	9.964	39.9	36.2
Fans and Polygons: ESP_014266_0925 ESP_014410_0925 (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
-87.3	167.	8.77	22.08	73.6	74.6
Megabreccia and Layered Deposits in Holden Crater: ESP_014443_1530 ESP_022724_1530 (Interval in Earth days: 646)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-26.6	325.	0.41	-14.1	35.4	33.6
South Polar Layered Deposits Exposed in Chasma Australe Wall: ESP_014360_0985 ESP_022694_0985 (Interval in Earth days: 649)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-81.3	95.8	-6.3	-20.6	70.7	65.3
	Page 715 of 885 (8,850 images)