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.

Starburst Araneiform Stereo:   ESP_013147_0980   ESP_013833_0980   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.8

76.1

24.7

8.862

59.7

63.3

Well Preserved 20 Kilometer Diameter Impact Crater:   ESP_013684_1455   ESP_020910_1455   (Interval in Earth days: 563)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.0

168.

-2.8

19.71

36.4

51.7

Layered Bedrock in Northeast Hellas Planitia:   ESP_013964_1490   ESP_020267_1490   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.7

82.9

1.84

19.77

34.9

58.9

Basal Exposure of South Polar Layered Deposits:   ESP_013791_1070   ESP_014134_1070   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

134.

8.74

-8.76

56.2

60.7

Valleys and Layering along Melas Chasma:   ESP_013561_1705   ESP_013983_1705   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.60

283.

-0.8

-18.8

40.4

37.5

East Slope of Asimov Crater Central Pit:   ESP_013189_1330   ESP_013835_1330   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.8

5.12

-5.7

20.37

43.1

39.0

Pitted and Fractured Surfaces in Southern Mojave Region:   ESP_014034_1870   ESP_014311_1870   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.105

327.

0.98

-24.4

43.1

41.9

Crater Wall with Gullies at Multiple Elevations in MOC Image E1101445:   ESP_013236_1410   ESP_013948_1410   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.7

159.

5.50

16.26

39.9

36.0

Active Geyser Locale:   ESP_014083_0945   ESP_014122_0945   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.4

103.

8.28

22.35

69.3

68.8

Central Uplift of a Large Impact Crater:   ESP_012988_1560   ESP_029893_1560   (Interval in Earth days: 1317)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

88.6

0

-20.0

43.5

51.7


  


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