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.

Banding at Margin of Circular Feature in CTX Image:   ESP_017534_1690   ESP_087596_1685   (Interval in Earth days: 5459)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.1

177.

-8.5

-24.7

60.5

60.6

Small Crater in Amazonis Planitia:   ESP_017361_1830   ESP_018073_1830   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.024

219.

-6.7

4.499

51.3

52.3

Polar Crater with Summer Ice:   ESP_017510_2465   ESP_017945_2465   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
66.39

99.7

-0.4

14.50

49.4

48.4

Central Peak of an Impact Crater:   ESP_017430_1910   ESP_018709_1910   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.63

134.

-8.9

4.868

48.0

49.4

Very Fresh Double Crater:   ESP_017613_2195   ESP_017903_2195   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.31

174.

-11.

8.67

42.6

41.3

Crater Cut by Horst and Graben:   ESP_017399_2185   ESP_017900_2185   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.10

256.

-4.2

10.29

41.5

41.1

Enigmatic Uplift on the Floor of Echus Chasma:   ESP_017306_1815   ESP_018084_1815   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.718

279.

5.93

-6.88

50.8

53.8

Circular Features in Far Northern Reaches of Arcadia Planitia:   ESP_017632_2475   ESP_018634_2475   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.05

9.22

-2.5

13.14

49.8

52.6

Streamlined Landform with Benches in Kasei Valles System:   ESP_017398_1970   ESP_017820_1970   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.92

285.

9.39

-8.3

43.9

46.4

Light-Toned Layered Deposits on Northern Edge of Hellas Planitia:   ESP_017459_1500   ESP_018870_1500   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.5

66.7

3.18

-25.8

72.3

72.8


  


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