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.

Phlegra Montes:   ESP_075346_2165   ESP_093055_2165   (Interval in Earth days: 1380)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.21

162.

7.16

-14.4

69.2

69.2

Scarp Monitoring:   ESP_075270_1190   ESP_075613_1190   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-60.7

92.0

-2.1

-18.0

48.1

50.6

Light-Toned Deposits in Iani Chaos:   ESP_075366_1795   ESP_075999_1795   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.28

341.

-1.3

-14.2

44.5

39.1

Canyon Floor in East Coprates Chasma:   ESP_075407_1650   ESP_075473_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.0

304.

-4.1

-21.8

38.2

39.0

Mounds and Pit on Thick Carbon Dioxide Ice:   ESP_075399_0920   ESP_074989_0920   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.1

219.

15.6

25.47

66.9

64.0

Layers at Edge of Pedestal Crater in Tikhonravov Crater:   ESP_075364_1940   ESP_076353_1940   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.64

35.2

-7.3

2.427

53.3

41.6

Distal Ramparts of Fresh Impact Crater:   ESP_075440_2035   ESP_083840_2035   (Interval in Earth days: 655)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.43

118.

4.11

17.21

58.5

62.6

Fractured Rises in Iani Chaos:   ESP_075445_1770   ESP_076434_1770   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.79

346.

-5.3

6.497

42.5

35.2

Volcanic Flow near Tempe Terra:   ESP_075487_2110   ESP_084177_2110   (Interval in Earth days: 677)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.56

275.

-5.0

7.021

63.8

64.8

Channel and Crater North of Huygens Crater:   ESP_075416_1745   ESP_075772_1745   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.39

57.5

0.14

18.63

41.3

36.4


  


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