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.

Pit in Hephaestus Fossae:   ESP_060260_2015   ESP_055209_2015   (Interval in Earth days: 393)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.35

127.

9.79

21.07

36.4

50.9

Pedestal Crater Near Phlegra Montes:   ESP_060417_2185   ESP_060351_2185   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.95

160.

-7.7

7.658

41.0

39.9

Fissure Adjacent to Olympica Fossae:   ESP_060282_2055   ESP_060427_2055   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.36

246.

1.79

18.58

37.4

36.2

Depressions in Arena Colles:   ESP_060301_2040   ESP_060789_2040   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.92

88.4

0.12

-18.9

37.5

40.6

Candidate Landing Site for 2020 Mission Near Jezero Crater:   ESP_060341_1985   ESP_060407_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.25

77.1

0.99

-18.2

37.5

39.5

Sinuous Gullies and Arcuate Ridges:   ESP_060214_1355   ESP_060280_1355   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.1

311.

8.88

-7.81

68.5

70.4

Sand Dune Changes in Hellespontus Region:   ESP_060224_1350   ESP_060290_1350   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.8

38.7

7.87

-8.66

69.3

71.1

Chaotic Terrain Near Ravi Vallis:   ESP_060451_1790   ESP_061018_1790   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.98

316.

6.53

26.02

43.5

47.1

Gullies:   ESP_060298_1340   ESP_060153_1340   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.5

178.

7.78

-7.22

70.8

69.5

Two Small Cones in Hydraotes Chaos:   ESP_060266_1795   ESP_060754_1795   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.34

326.

6.09

-16.5

41.3

47.7


  


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