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.

A Slice through the Layercake:   ESP_084979_1975   ESP_085045_1975   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.49

336.

16.6

-4.34

44.6

45.3

North Pole Facing Deposit in Crater:   ESP_085774_2230   ESP_085853_2230   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.65

234.

0.49

23.69

53.0

50.5

Avalanches on Walls of Gully in Echus Fossae:   ESP_085957_1810   ESP_086880_1810   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.056

282.

3.62

-19.7

38.1

47.9

Exposure of Layered Materials along Hellas Planitia Rim Escarpment:   ESP_085807_1590   ESP_086242_1590   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.7

63.1

-16.

0.443

44.6

49.5

Raised Circular Feature:   ESP_085811_2210   ESP_086246_2210   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.81

305.

-6.0

6.055

51.8

47.1

Gullied Slope:   ESP_085723_1370   ESP_085868_1370   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.8

197.

-4.7

10.24

55.4

56.9

Kasei Valles Lava:   ESP_085970_1965   ESP_086326_1965   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.39

285.

4.76

-6.69

38.9

40.3

Giant Polygon Terminus:   ESP_085849_2205   ESP_086996_2205   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.92

346.

2.02

17.45

50.4

42.0

Kasei Valles Lava:   ESP_085825_1965   ESP_085614_1965   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.14

285.

4.28

-6.99

39.1

40.5

Hillslope Morphologies in Crater:   ESP_085793_1510   ESP_086294_1510   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

84.7

3.79

-4.91

47.1

55.3


  


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