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.

South Polar Layered Deposits :   ESP_057906_0925   ESP_057891_0925   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.5

54.9

2.46

13.98

69.5

67.4

High-Latitude Exposure of South Polar Layered Deposits :   ESP_057902_0875   ESP_057888_0875   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.3

204.

8.96

1.928

70.7

70.1

Exposure of South Polar Layered Deposits :   ESP_058100_0915   ESP_057624_0915   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

122.

19.8

27.08

70.4

65.0

Terrain in Lyot Crater :   ESP_058035_2295   ESP_058101_2295   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.88

30.3

8.51

-7.35

73.2

73.1

Candidate Recent Impact Site :   ESP_058220_1945   ESP_075272_1945   (Interval in Earth days: 1329)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.33

24.6

3.28

15.56

43.5

53.5

Possible Exposure of South Polar Layered Deposits :   ESP_058087_0915   ESP_057640_0915   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.5

106.

23.2

16.57

69.9

66.6

Stratigraphy in Ius Chasma Region :   ESP_058079_1720   ESP_058725_1720   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.95

278.

-4.7

6.876

33.2

29.8

Possible Olivine-Rich Terrain :   ESP_057902_1570   ESP_058680_1570   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.7

70.6

4.04

-15.5

30.8

33.4

Gullies Monitoring :   ESP_058049_1275   ESP_058115_1275   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.1

23.0

3.26

-14.7

41.7

43.4

Floor of East Candor Chasma :   ESP_057973_1735   ESP_057907_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.47

291.

-8.4

5.757

35.0

34.7


  


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