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

Zhurong Rover Landing Site Region: ESP_077722_2055 ESP_077788_2055 (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
25.36	109.	-5.0	-25.8	41.9	43.9
Dune Changes near Martz Crater: ESP_077629_1420 ESP_077919_1420 (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
-37.7	136.	4.84	19.09	63.4	66.9
Channels Intersecting Crater in Xanthe Terra: ESP_077702_1755 ESP_076805_1755 (Interval in Earth days: 70)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.60	301.	-27.	-7.96	47.8	37.6
Region East of Medusae Fossae: ESP_077534_1790 ESP_078180_1790 (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
-1.19	206.	0.00	11.53	42.6	48.2
Monitor Gullies and Lobes in Can Crater : ESP_077555_2285 ESP_077344_2285 (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
48.21	345.	4.73	-6.81	50.4	53.1
Crater in Arabia Terra: ESP_077607_2180 ESP_078029_2180 (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
37.81	5.52	19.9	-4.06	43.7	44.1
Looking at the Crater Half Full: ESP_076968_1475 ESP_076823_1475 (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
-32.4	173.	23.4	-6.17	48.0	47.6
Crater: ESP_077219_1455 ESP_085157_1455 (Interval in Earth days: 618)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-34.1	167.	-6.1	-22.1	55.1	42.9
Lava in Kasei Valles: ESP_077122_2025 ESP_077399_2025 (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
22.09	286.	-4.9	5.772	41.7	40.4
Northern Chaos Terrain as Source for Outflow into Osuga Valles: ESP_077121_1640 ESP_076712_1640 (Interval in Earth days: 32)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-16.0	319.	-17.	7.426	44.6	37.8
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