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.

Surface Features of Debris Apron in Deuteronilus Mensae :   ESP_046787_2210   ESP_090199_2210   (Interval in Earth days: 3382)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.80

23.8

7.56

-18.2

62.6

59.2

Small Dome and Barchan Dunes in Newton Crater :   ESP_046649_1385   ESP_046504_1385   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.1

202.

2.56

-11.2

62.5

65.3

Candidate Recent Impact Site :   ESP_046707_2220   ESP_055146_2220   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.45

48.7

-1.4

-21.1

62.4

59.2

Youthful Dark Rayed Crater with Boulders in Primary Ejecta Deposit :   ESP_046618_1770   ESP_047330_1770   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.07

324.

-8.1

2.309

52.2

51.0

Northern Ejecta and Rays of Istok Crater :   ESP_046686_1350   ESP_064580_1350   (Interval in Earth days: 1394)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.8

274.

-5.2

19.11

64.4

62.9

Monitor Seasonal Changes at South Polar Cracked and Gullied Site :   ESP_046892_0980   ESP_046945_0980   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.6

66.2

4.68

-8.76

81.2

81.2

Lava Crust and Wakes in Amazonis Planitia :   ESP_046675_2090   ESP_064002_2090   (Interval in Earth days: 1350)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.74

204.

-7.0

15.14

57.2

56.2

Possible Phyllosilicates in Knob-Type Feature North of Hellas Planitia :   ESP_046601_1580   ESP_064706_1580   (Interval in Earth days: 1411)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.9

71.1

-5.0

21.42

55.8

55.7

Cratered Layered Terrain and Wall Slopes in Melas Chasma :   ESP_046725_1685   ESP_046448_1685   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.2

285.

-11.

16.82

53.1

51.8

Ice-Rich Deposits in Ancient Valleys :   ESP_046716_1415   ESP_064742_1415   (Interval in Earth days: 1405)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

172.

6.21

-3.51

60.1

60.2


  


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