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

Cataracts in Kasei Valles : PSP_002814_2055 PSP_003513_2055 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.07	298.	4.29	-26.3	60.8	68.0
North Flank of Apollinaris Patera: PSP_001645_1725 PSP_002634_1725 (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
-7.40	174.	4.03	29.14	57.3	53.4
Dissected Wall of Mojave Crater: PSP_001481_1875 PSP_002167_1880 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.783	326.	3.49	-17.4	51.7	55.6
Crater and Extensive Field of Secondary Craters Seen in MOC Image R15-02146: PSP_002230_1850 ESP_027890_1850 (Interval in Earth days: 1999)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.727	46.1	-7.8	4.118	55.2	51.4
Dark-Toned Unit Exposed atop Crater Ejecta in Meridiani Planum : PSP_002680_1825 PSP_003392_1825 (Interval in Earth days: 55)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.240	-0.3	7.78	29.45	55.2	53.5
Fresh Impact Crater with Bright, Rocky Ejecta: PSP_001782_1655 PSP_002204_1655 (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
-14.1	38.6	2.21	-11.5	60.0	59.5
Rayed Crater: PSP_001660_1950 PSP_002570_1950 (Interval in Earth days: 71)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
14.87	123.	-1.8	-15.8	51.1	57.9
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
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
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
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