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.

Extensive Boxwork in Terra Sabaea:   ESP_084634_1525   ESP_092084_1525   (Interval in Earth days: 580)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.0

44.2

0.44

-13.1

35.3

47.5

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084894_1050   ESP_084762_1050   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.0

156.

-0.7

14.00

65.3

62.6

Channels near Moreux Crater:   ESP_084726_2205   ESP_093547_2205   (Interval in Earth days: 687)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.33

43.5

-4.4

26.32

65.6

63.7

Layered Bedrock and Bedforms in Flaugergues Crater:   ESP_084648_1625   ESP_091966_1625   (Interval in Earth days: 570)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.3

20.9

-3.2

23.19

35.0

47.4

Overlapping Debris Aprons within Ganges Chasma:   ESP_084848_1720   ESP_085138_1720   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.01

318.

-8.1

20.34

36.1

33.3

Gullies with Long Channels in Sisyphi Cavi:   ESP_084781_1095   ESP_091756_1095   (Interval in Earth days: 543)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-70.4

-1.1

1.26

29.95

60.1

60.2

Small Scale Lobes on Isolated Mound:   ESP_084819_1045   ESP_093007_1045   (Interval in Earth days: 638)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.1

42.8

5.81

27.72

64.0

55.8

Tectonics on Northern Coprates Chasma Wall:   ESP_084506_1670   ESP_084585_1670   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.6

299.

-16.

14.14

37.5

34.7

Channels in Hellas Planitia:   ESP_084792_1490   ESP_085570_1490   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

50.7

-6.9

8.445

37.3

44.7

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084655_1000   ESP_084971_1000   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.0

208.

-0.0

24.15

65.9

69.1


  


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