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

Lava Flow Margin in Amazonis Planitia: PSP_008804_2055 PSP_009226_2055 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.51	192.	6.80	-18.1	43.1	46.4
Layered Rocks in Northern Hellas Planitia: PSP_008756_1510 PSP_008967_1510 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.8	69.8	7.46	-14.8	72.4	74.3
High-Latitude Exposure of North Polar Layered Deposits: PSP_009263_2675 PSP_009370_2675 (Interval in Earth days: 8)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.49	182.	-3.5	-13.3	62.9	63.2
Transition between Medusae Fossae Formation and Clusters of Aligned Cones: PSP_009175_1810 PSP_009808_1810 (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
1.222	145.	-2.2	-24.0	54.7	57.1
Tube-Fed Lava Flow Field: PSP_008433_1755 PSP_009501_1755 (Interval in Earth days: 83)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.58	247.	7.65	-15.8	54.7	59.2
Crater Floor and Central Mound in Gale Crater (MSL): PSP_009505_1755 PSP_009571_1755 (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
-4.47	137.	-7.4	-28.4	58.6	60.2
High-Latitude Exposure of North Polar Layered Deposits: PSP_009243_2675 PSP_009297_2675 (Interval in Earth days: 4)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
87.62	13.0	-5.1	-13.9	62.9	63.0
Dark Materials on Block in Olympus Mons Aureole: PSP_008935_1975 ESP_016372_1975 (Interval in Earth days: 580)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.33	217.	-8.1	5.979	47.1	40.0
Arcadia Planitia Domes: PSP_008554_2170 PSP_008765_2170 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
36.67	177.	4.87	-13.3	41.4	43.3
Textured Plain in Arcadia Planitia: PSP_008566_2285 ESP_016069_2285 (Interval in Earth days: 585)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
48.18	209.	-4.0	-26.0	43.4	49.7
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