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

Channel Entering Sklodowska Crater: ESP_088512_2130 ESP_088578_2130 (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
32.92	358.	15.6	-3.74	42.6	44.5
Kasei Valles Alluvial Fans: ESP_088633_2040 ESP_088778_2040 (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
23.55	298	-6.4	3.817	46.5	46.1
Pitted Cones with Moat near Potential Volcano: ESP_088416_2080 ESP_088627_2080 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
27.47	102.	-6.6	-18.5	45.1	46.7
Channels along Hydraotes Chaos Channel: ESP_088566_1835 ESP_088711_1835 (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
3.377	329.	3.41	14.35	53.8	53.2
Gullies on Western Wall of Nier Crater: ESP_088574_2230 ESP_088640_2230 (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
42.77	105.	-0.5	-17.0	44.0	45.8
Lobate Glacial Deposit in Crater: ESP_088601_2150 ESP_088825_2150 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
34.85	90.4	-8.8	26.07	44.8	42.4
Jezero Crater: ESP_088562_1985 ESP_089208_1985 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.47	77.4	-8.9	15.11	48.1	47.9
Dune Monitoring in Northern Mid-Latitude Crater: ESP_088500_2435 ESP_088421_2435 (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
62.98	320.	7.80	-6.45	48.1	49.1
Alluvial Fans and Terraced Scarps in Kasei Valles: ESP_088541_2025 ESP_088330_2025 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
22.38	291.	-19.	-6.13	47.7	46.0
Wrinkle Ridge and Valley Network Intersection: ESP_088616_1750 ESP_088471_1750 (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
-4.96	45.5	-4.8	-15.5	59.1	59.6
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