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

Debris Flow: ESP_020558_2215 ESP_020835_2215 (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
41.17	50.8	-3.6	-22.7	69.0	73.7
Possible Olivine in East Thaumasia Planum: ESP_020905_1525 ESP_083306_1525 (Interval in Earth days: 4862)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.0	305.	4.56	13.84	52.0	45.6
Central Structure of Large Impact Crater: ESP_020695_1440 ESP_029398_1440 (Interval in Earth days: 678)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-35.5	280.	-0.9	26.38	56.6	55.8
Potential Future Mars Landing Site in Mawrth Region: ESP_020442_2055 ESP_029277_2055 (Interval in Earth days: 688)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
25.26	339.	2.82	-6.15	60.5	60.9
Bedrock Exposure in Landslide Scarp: ESP_020879_1670 ESP_021657_1670 (Interval in Earth days: 61)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-12.9	293.	5.19	-7.68	52.2	46.1
Faulted Crater in Claritas Rupes: ESP_020564_1455 ESP_020841_1455 (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
-34.2	256.	4.03	-21.5	57.7	56.0
Eroded Pitted Materials on Floor 90-Kilometer Diameter Impact Crater: ESP_020553_1650 ESP_020698_1650 (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
-14.6	193.	5.79	20.85	54.1	52.0
Central Uplift with Tilted Layers: ESP_020734_1540 ESP_021578_1540 (Interval in Earth days: 65)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-25.7	293.	6.48	-23.2	53.7	45.8
Heavily Pitted Streamlined Ejecta Lobe Originating from Mojave Crater: ESP_020548_1875 ESP_028539_1875 (Interval in Earth days: 623)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
7.169	328.	-7.9	11.85	56.9	51.8
Well-Preserved 3-Kilometer Diameter Impact Crater in Terra Sirenum: ESP_020725_1525 ESP_029283_1525 (Interval in Earth days: 667)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-27.3	179.	6.77	24.62	53.9	54.9
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