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

Layered Outcrops : ESP_029514_1820 ESP_030292_1820 (Interval in Earth days: 60)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
2.124	350.	3.30	-11.2	54.8	53.9
Mound and Textured Material in THEMIS Image I08552017 in Hydraotes Chaos : ESP_029660_1780 ESP_037743_1780 (Interval in Earth days: 630)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-1.89	325.	-1.6	14.37	54.2	55.6
Grjota Valles Constriction : ESP_029468_1920 ESP_037617_1920 (Interval in Earth days: 635)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
11.83	165.	3.37	-10.4	57.1	56.8
Monitoring Active Dunes in Arabia Terra : ESP_029605_1815 ESP_029961_1815 (Interval in Earth days: 28)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
1.219	26.4	1.11	12.56	54.8	53.3
Source Area for Channel Network Near Gigas Sulci : ESP_029716_1980 ESP_029426_1980 (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
17.81	232.	15.8	-10.3	59.5	59.8
Light-Toned Depostis Along Coprates Chasma Floor : ESP_029595_1660 ESP_047054_1660 (Interval in Earth days: 1360)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-13.9	301.	1.95	10.85	52.7	50.3
Colorful Fractured Bedrock in Ritchey Crater: ESP_029542_1510 ESP_029964_1510 (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
-28.5	308.	14.3	3.043	53.3	49.1
Impacts from MSL Tungsten Blocks and Cruise Stage: ESP_029245_1755 ESP_031869_1755 (Interval in Earth days: 204)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-4.40	136.	1.29	-18.0	54.3	35.6
Columnar Jointing on Mars and Earth: ESP_029286_1885 ESP_030143_1885 (Interval in Earth days: 67)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
8.599	95.5	-3.4	18.28	56.1	55.5
Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor : ESP_029103_1675 ESP_029037_1675 (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
-12.5	54.0	-1.6	21.19	55.5	53.9
	Page 518 of 873 (8,724 images)