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.

Interesting Landslide Morphology and Phyllosilicate Detections :   ESP_044871_1740   ESP_043961_1740   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.17

137.

7.69

21.68

54.3

53.3

Pasted-on Material on Crater Ejecta :   ESP_044720_1890   ESP_045353_1890   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.847

299.

-8.8

8.465

47.6

46.2

Pits Fissures and Channels East of Olympus Mons :   ESP_044841_1960   ESP_044907_1960   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.86

233.

6.54

-11.9

43.6

45.1

Candidate ExoMars Landing Site in Oxia Palus :   ESP_044824_1985   ESP_062481_1985   (Interval in Earth days: 1376)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.08

336.

23.1

5.898

41.5

45.8

Double-Terraced Crater in Arcadia Planitia :   ESP_044724_2270   ESP_044869_2270   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.75

183.

5.44

19.31

41.4

40.8

Possible Phyllosilicates in Knobs within Depression on Dichotomy Boundary :   ESP_044995_2165   ESP_052023_2165   (Interval in Earth days: 548)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.32

347.

7.00

27.66

41.0

36.1

Southwestern Elysium Planitia :   ESP_044963_1815   ESP_045385_1815   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.457

146.

-1.1

12.18

50.5

48.9

Fractured Surface Near Athabasca Valles Lava :   ESP_044831_1825   ESP_053560_1825   (Interval in Earth days: 680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.431

148.

3.35

17.54

49.8

49.5

North Polar Layered Deposits 160-Meter Diameter Crater Monitoring :   ESP_044810_2620   ESP_044784_2620   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.84

333.

7.95

-6.74

59.0

59.6

Meridiani Planum :   ESP_044718_1780   ESP_046274_1780   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.19

354.

2.37

19.53

52.6

49.7


  


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