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.

Channel Bedforms and Fan North of Arabia Terra:   ESP_068533_2195   ESP_078173_2195   (Interval in Earth days: 751)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.35

33.9

4.61

-7.92

50.5

44.5

Impact Crater adjacent to Ravine:   ESP_068867_1985   ESP_078823_1985   (Interval in Earth days: 776)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.09

288.

1.03

12.18

45.8

44.6

Modification of Small Terraced Crater:   ESP_068829_2480   ESP_069251_2480   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.82

233.

4.32

25.32

62.9

57.0

Very Well-Preserved 900-Meter Northern Plains Crater :   ESP_068700_2420   ESP_068687_2420   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.49

155.

-0.2

-26.2

60.9

63.1

Cones in Tharsis Region:   ESP_068895_1890   ESP_069093_1890   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.120

243.

26.6

2.819

44.7

48.4

Crater Gullies at Multiple Elevations:   ESP_067299_1435   ESP_067708_1435   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.1

227.

-6.6

3.913

42.9

47.4

Layered Deposits on South Wall of West Candor Chasma:   ESP_068392_1730   ESP_076832_1730   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.96

284.

21.9

0.965

43.9

37.3

Eos Chasma Slumps:   ESP_068444_1630   ESP_067718_1630   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

310.

-18.

14.65

51.0

39.5

Streamlined Form in Kasei Valles:   ESP_068326_1990   ESP_069474_1990   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.78

283.

-7.8

6.899

45.0

48.4

Modified Fan in Shalbatana Vallis:   ESP_068457_1760   ESP_078598_1760   (Interval in Earth days: 790)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.18

313.

-0.6

22.00

45.7

52.6


  


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