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.

Candidate Landing Site in a Possible Salt Playa:   ESP_016288_1745   ESP_016433_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.64

353.

0.58

17.63

47.4

47.7

Layering in Hellas Planitia:   ESP_016299_1420   ESP_019978_1420   (Interval in Earth days: 287)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.4

57.0

7.21

-12.1

67.3

67.2

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

Central Peak of 70-Kilometer Diameter Impact Crater in Terra Sabaea:   ESP_016114_1580   ESP_016470_1580   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.9

66.7

-6.2

4.62

55.0

58.8

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

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

Layers North of Hellas Planitia with Strong Phyllosilicate Signature:   ESP_016259_1535   ESP_016404_1535   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.4

67.6

6.31

21.54

59.1

60.0

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

Clays and Chlorides in Sirenum Region:   ESP_016043_1480   ESP_016188_1480   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.6

206.

-5.5

9.37

60.3

61.5


  


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