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

Gullies : PSP_002283_1335 PSP_002560_1335 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-45.9	45.7	-3.5	-23.7	71.7	69.6
Location of Possible Very Recent Gully Activity: PSP_002040_1435 PSP_002185_1435 (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
-36.3	198.	-3.0	11.28	69.4	67.0
Light-Toned Layered Material in South Galle Crater : PSP_002866_1280 ESP_064565_1280 (Interval in Earth days: 4808)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-51.8	329.	1.76	-20.3	65.6	68.7
Layered Deposit in a Small Crater within Schiaparelli Crater: PSP_002363_1800 PSP_002508_1800 (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
-0.18	14.4	7.82	23.78	54.7	53.5
Ganges Mensa : PSP_002550_1725 PSP_003618_1725 (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
-7.25	311.	-4.4	26.16	56.4	49.8
Eastern Rim and Ejecta of Tomini Crater: PSP_002227_1965 ESP_055486_1965 (Interval in Earth days: 4151)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
16.25	125.	0	23.73	54.3	52.1
Channels South of the Base of Ascraeus Mons: PSP_001985_1860 PSP_002486_1860 (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
5.998	254.	-3.9	22.18	54.0	53.5
Low-Latitude North Polar Layered Deposits and Basal Unit Contact: PSP_001548_2755 PSP_001694_2755 (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
84.4	142.	1.30	17.73	75.0	74.8
Gullies: PSP_002266_2190 PSP_002411_2190 (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
38.55	137.	7.46	18.68	58.2	59.3
Eroded Layers and Scallops and Polygons: PSP_001964_2275 PSP_003177_2275 (Interval in Earth days: 95)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
46.94	101.	-0.2	25.63	57.3	73.4
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