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

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
Possible Phoenix Lander Landing Site: TRA_000881_2475 TRA_000894_2475 (Interval in Earth days: 1)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
67.49	130.	-21.	0	54.9	53.3
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
Interior Channel in Parana Valles: PSP_002008_1560 PSP_002285_1560 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.9	350.	-0.6	-27.3	63.5	63.7
Dark Materials on Block in Olympus Mons Aureole : PSP_002461_1975 ESP_011282_1975 (Interval in Earth days: 687)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.06	217.	-4.5	16.43	56.5	56.4
Tooting Crater West Rim and Ejecta : PSP_002580_2035 PSP_002646_2035 (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
23.15	207.	3.51	-16.7	58.0	60.3
Tooting Crater Interior: PSP_001538_2035 PSP_002158_2035 (Interval in Earth days: 48)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
23.18	207.	23.1	11.74	47.1	53.3
Gullies in Dark Layers in Crater Wall: PSP_002212_1335 PSP_002291_1335 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-46.2	184.	-6.7	21.92	73.0	70.0
Potential Lobe of Lahar Flow Front: PSP_002042_2090 PSP_002108_2090 (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
28.85	134.	5.87	-13.1	53.3	55.7
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
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