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.

Gale Crater Rim Deposits:   ESP_022045_1745   ESP_022190_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.43

138.

4.26

18.22

43.9

41.2

Bedrock in Central Peak of Crater on North Rim of Hellas Basin:   ESP_022245_1485   ESP_022746_1485   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.3

81.6

4.98

25.98

35.4

31.2

Possible MSL Rover Landing and Seismic Network Site in Utopia Region:   ESP_022178_1960   ESP_022534_1960   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.61

105.

-3.8

4.541

55.5

50.9

Inverted Valleys near Juventae Chasma:   PSP_007627_1765   PSP_008563_1765   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.67

297.

-4.8

5.755

48.7

55.0

Possible Inverted Topography Landscape with Clay Minerals:   ESP_022077_2000   ESP_022367_2000   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.80

342.

-1.5

22.08

59.3

54.9

Bedform Changes in Aureum Chaos:   ESP_021906_1765   ESP_022183_1765   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.64

333.

-1.9

-28.1

46.7

45.5

Candidate New Gully Flow Formed between 15 May 2009 and 3 March 2011:   ESP_021914_1475   ESP_022336_1475   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.3

118.

3.26

-10.0

39.2

35.9

Light-Toned Sedimentary Rocks Exposed in Syrtis Major Region Scarp:   ESP_021757_1975   ESP_021612_1975   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.13

76.7

23.0

12.29

58.4

59.8

Crater with Channel-Like Feature:   ESP_021907_1710   ESP_022329_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.79

307.

-6.2

-20.3

44.7

40.7

Lobate Crater Fill in Southeast Hellas Montes:   ESP_021809_1385   ESP_021743_1385   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.2

106.

6.08

23.72

41.4

40.8


  


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