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.

Bright Layers in Columbus Crater:   ESP_016083_1505   ESP_016584_1505   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

193.

-4.3

21.15

59.1

63.9

Sinuous Ridges in the Aeolis and Zephyria Regions:   ESP_016282_1750   ESP_016915_1750   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.04

155.

22.5

8.613

45.4

52.2

Crater Rim Gullies Filled with Small Dunes:   ESP_015934_2165   ESP_037243_2165   (Interval in Earth days: 1660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.09

292.

1.58

-16.4

42.8

56.6

Massif with Radial Troughs in Viking 072A02:   ESP_016011_2185   ESP_016499_2185   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.06

347.

25.6

2.429

41.2

41.5

Layered Bedrock in Central Uplift of a Large Crater:   ESP_016132_1595   ESP_016765_1595   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.3

293.

8.27

-7.22

53.3

61.6

Gullied Crater Wall:   ESP_016191_1415   ESP_026951_1415   (Interval in Earth days: 838)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.1

125.

6.43

-7.63

66.4

79.4

Deep Bedrock Exposure in Melas Chasma:   ESP_016264_1705   ESP_016897_1705   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.22

288.

7.41

-7.19

48.5

55.6

Unusual Flow-Ejecta Morphology:   ESP_016226_1480   ESP_016371_1480   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.7

249.

5.73

20.76

62.3

63.3

Bedrock Exposed by Impact Crater:   ESP_016275_1535   ESP_016420_1535   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.1

350.

8.04

23.11

59.0

59.8

Kunowsky Crater Central Peak with Strong Olivine Signature:   ESP_016235_2370   ESP_016314_2370   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.79

350.

8.37

25.32

50.4

48.5


  


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