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 and Chlorides in Hadriacus Cavi:   ESP_084000_1525   ESP_084580_1525   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

77.5

0.48

16.98

38.3

34.0

Interaction of Fluvial Ridge with Kilometer-Scale Polygonal Ridge System:   ESP_083739_1990   ESP_084029_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.93

0.25

-15.

-5.08

62.5

58.8

Unit Margin and Pit:   ESP_083989_1115   ESP_084121_1115   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-68.3

25.5

4.01

-20.4

52.2

54.0

Gullied Slope Monitoring:   ESP_083426_1325   ESP_083492_1325   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.2

274.

-0.2

-14.4

46.9

47.1

Channels and Fan in Crater in Aeolis Region:   ESP_083470_1800   ESP_083681_1800   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.02

146.

-0.2

-17.8

52.8

51.8

West Hellespontus Complex Dune Field:   ESP_083342_1395   ESP_083909_1395   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.1

45.1

7.14

-8.63

46.1

40.8

Very Fresh Crater in Terra Sabaea:   ESP_083645_1610   ESP_083711_1610   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.0

49.6

10.0

-18.5

42.9

44.2

Crater and Banded Terrain in Hellas Planitia:   ESP_083434_1400   ESP_083500_1400   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

53.8

5.77

-9.88

44.8

45.2

Landslide on Crater Wall:   ESP_083410_1935   ESP_083344_1935   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.28

341.

7.82

25.40

60.0

59.1

Linear Ridges Intersecting Valley Topography:   ESP_083580_1530   ESP_083514_1530   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

28.7

-23.

0.494

45.0

43.9


  


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