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

Light and Layered Crater Fill Material in Flaugergues Crater: ESP_016142_1625 ESP_016775_1625 (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
-17.4	20.8	5.06	-10.3	51.9	60.0
Layers in Trough Floor and Scarp of Western Bench of Terby Crater: ESP_016206_1525 ESP_016351_1525 (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
-27.4	74.5	8.70	23.26	59.0	59.9
Bedrock Exposed by Impact Crater: ESP_016275_1535 ESP_016420_1535 (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
-26.1	350.	8.04	23.11	59.0	59.8
Crescentic Scour Features in Mff: ESP_016254_1830 ESP_016399_1830 (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
2.753	201.	-8.2	8.768	44.1	44.0
Possible MSL Landing Site in Holden Crater: ESP_015999_1535 ESP_016276_1535 (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
-26.4	325.	13.9	-13.6	55.0	60.5
Bedrock Exposures in Wall of Impact Crater: ESP_016152_2115 ESP_017075_2115 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
31.01	102.	-1.6	10.61	40.8	40.0
Stranded Lobe of Material with Associated Ridge on Valley Floor: ESP_016238_2180 ESP_017161_2180 (Interval in Earth days: 72)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
37.54	273.	-3.4	6.789	42.5	40.5
Stratigraphic Relations in MOC Image M00-02426 in Sinus Meridiani: ESP_016169_1790 ESP_019637_1790 (Interval in Earth days: 270)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-0.77	1.73	4.18	-16.4	43.8	56.0
Massif in Deuteronilus Mensae: ESP_016141_2260 ESP_016431_2260 (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
45.44	39.7	3.75	23.76	45.5	42.2
Gullied Slope of 20-Kilometer Diameter Impact Crater in Acidalia Planitia: ESP_016170_2230 ESP_016460_2230 (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
42.64	329.	0.01	21.35	44.4	41.3
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