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.

Layers in Trough Floor and Scarp of Western Bench of Terby Crater:   ESP_016206_1525   ESP_016351_1525   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.4

74.5

8.70

23.26

59.0

59.9

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

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

Athabasca Valles:   ESP_016071_1890   ESP_024708_1890   (Interval in Earth days: 673)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.934

155.

7.83

-16.8

39.6

38.8

Crescentic Scour Features in Mff:   ESP_016254_1830   ESP_016399_1830   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.753

201.

-8.2

8.768

44.1

44.0

Possible MSL Landing Site in Holden Crater:   ESP_015999_1535   ESP_016276_1535   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.4

325.

13.9

-13.6

55.0

60.5

Bedrock Exposures in Wall of Impact Crater:   ESP_016152_2115   ESP_017075_2115   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.01

102.

-1.6

10.61

40.8

40.0

Stranded Lobe of Material with Associated Ridge on Valley Floor:   ESP_016238_2180   ESP_017161_2180   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.54

273.

-3.4

6.789

42.5

40.5

Massif in Deuteronilus Mensae:   ESP_016141_2260   ESP_016431_2260   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.44

39.7

3.75

23.76

45.5

42.2

Fresh Impact Crater in Northern Plains:   ESP_016164_2170   ESP_016797_2170   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.79

133.

4.17

-6.96

41.9

41.7


  


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