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.

Yardangs in Aeolis Region:   ESP_082204_1800   ESP_082336_1800   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.07

151.

6.30

-25.1

57.9

60.5

Lava Interactions with Landscape:   ESP_082228_1545   ESP_082663_1545   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

221.

-7.6

21.04

60.0

53.2

Hematite-Rich Terrain in West Candor Chasma:   ESP_082120_1745   ESP_082331_1745   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.24

285.

-1.4

12.00

58.3

56.8

Volcanic Vent East of Pavonis Mons:   ESP_082174_1795   ESP_082240_1795   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.46

251.

-3.3

-20.3

58.6

60.0

Hillslope Morphologies in Crater:   ESP_082342_1655   ESP_090372_1655   (Interval in Earth days: 626)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

347.

3.30

-13.1

57.2

61.3

Banded Terrain and Layering in Hellas Planitia:   ESP_082221_1400   ESP_082366_1400   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.9

53.0

6.65

29.05

62.6

58.7

Lava-Topography Interactions:   ESP_082294_1535   ESP_082162_1535   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.4

221.

-23.

8.101

60.8

59.7

Layered Margin of Mesa near Mawrth Vallis:   ESP_082184_2035   ESP_082619_2035   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.46

335.

-6.6

25.25

63.7

64.3

Light-Toned Mesas near Mawrth Vallis:   ESP_082395_2040   ESP_074074_2040   (Interval in Earth days: 648)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.60

336.

-0.5

-23.0

65.0

68.7

Two-Toned Bedrock Exposed in 5-Kilometer Crater in Noachis Terra:   ESP_082144_1480   ESP_082078_1480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.8

354.

-8.4

7.7

62.4

61.9


  


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