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

Megabreccia in Toro Crater: PSP_007767_1970 PSP_009270_1970 (Interval in Earth days: 117)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.01	71.8	-4.1	-18.6	42.2	49.0
Candidate Landing Site in NE Syrtis Major: ESP_015942_1980 ESP_016443_1980 (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
17.81	77.1	0	23.46	38.8	38.6
Colorful Streaks: ESP_016136_1525 ESP_020105_1525 (Interval in Earth days: 310)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.1	185.	5.15	16.28	58.0	59.5
The Dark Spot on Mars: ESP_013951_1955 ESP_020254_1955 (Interval in Earth days: 491)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
15.51	72.8	-7.7	11.92	49.9	55.5
Proposed MSL Landing Site in Eberswalde Crater: ESP_013533_1560 ESP_020891_1560 (Interval in Earth days: 574)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.8	327.	25.1	7.841	34.9	51.7
Southeastern Margin of Athabasca Valles: ESP_014304_1895 ESP_020185_1895 (Interval in Earth days: 458)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
9.148	156.	-6.5	24.68	41.7	53.0
Pebas Crater with Asymmetric Flow-Ejecta in Eastern Meridiani Planum: ESP_014389_1775 ESP_020692_1775 (Interval in Earth days: 491)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.59	-0.8	-27.	-14.9	37.7	55.8
Unnamed Fresh Crater South of Isidis Region: ESP_014412_1780 ESP_020715_1780 (Interval in Earth days: 491)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.06	88.9	-2.7	11.81	35.7	53.7
Channels from Hale Crater: PSP_005609_1470 PSP_005754_1470 (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
-32.5	320.	-8.1	6.815	37.6	38.1
Eroded Layered Deposits Near Ismenius Lacus: ESP_014414_2205 ESP_019728_2205 (Interval in Earth days: 414)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
40.40	29.2	-6.0	11.32	61.8	55.9
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