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

Inlet Valley: ESP_069653_1990 ESP_071011_1990 (Interval in Earth days: 106)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.77	78.3	9.32	24.07	49.2	48.0
Landforms in Utopia Planitia: ESP_069837_2120 ESP_070127_2120 (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
31.68	95.0	-8.5	6.367	48.8	47.0
Exposed Cliff of Stratified Deposits in Melas Chasma: ESP_069751_1670 ESP_070041_1670 (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
-12.8	287.	0.04	17.69	64.1	64.2
Possible Geological Contact Between Two Units: ESP_069685_1735 ESP_069342_1735 (Interval in Earth days: 27)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-6.56	289.	-3.1	7.599	60.5	56.3
Mounds in Western Oxia Colles: ESP_069802_2005 ESP_069657_2005 (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
20.16	330.	8.76	-7.69	49.3	50.3
Hill Southeast of Jezero Crater: ESP_069719_1985 ESP_070365_1985 (Interval in Earth days: 51)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.19	78.2	-3.7	7.67	50.8	50.0
Gully Monitoring and Topography: ESP_069895_2350 ESP_070528_2350 (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
54.55	305.	5.90	-17.6	49.5	49.6
Scalloped Depressions in Utopia Planitia: ESP_069692_2290 ESP_069982_2290 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
48.45	90.9	-4.2	10.12	49.7	47.4
Channel and Crater in Rahway Valles: ESP_069755_1910 ESP_070177_1910 (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
10.90	174.	13.4	-18.2	51.7	54.8
Recent Crater on Northern Plains: ESP_069968_2390 ESP_069889_2390 (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
58.81	110.	9.20	-6.73	50.1	51.9
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