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.

Streamlined Landforms in THEMIS Image V27359007:   ESP_032745_1415   ESP_032811_1415   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

341.

19.2

0.849

47.9

50.1

Gullies in Pit Wall:   ESP_032652_1300   ESP_024226_1300   (Interval in Earth days: 656)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.8

3.92

1.38

-19.6

55.6

63.1

Layered Materials on Northeast Hellas Region Rim:   ESP_032636_1525   ESP_032781_1525   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

78.1

-7.4

7.913

41.3

42.4

Fractured Ground in Arabia Terra:   ESP_032770_2155   ESP_032915_2155   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.15

11.8

-6.6

4.794

48.1

45.9

Valley Headwalls:   ESP_032743_2205   ESP_032888_2205   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.04

26.1

11.6

21.84

50.5

48.2

Light-Toned Stratified Materials in Melas Chasma:   ESP_032747_1690   ESP_033169_1690   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.5

285.

-2.6

-24.4

35.6

42.1

Very Well-Preserved Crater in Ares Vallis:   ESP_032521_1955   ESP_032943_1955   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.35

331.

8.89

-7.24

37.8

37.5

Large Dated Impact Crater:   ESP_032881_1855   ESP_032736_1855   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.457

224.

2.57

-13.9

34.8

35.7

Bright Dunes South of Echus Chasma:   ESP_032734_1780   ESP_058804_1780   (Interval in Earth days: 2031)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.00

279.

-8.6

20.37

34.8

29.5

USGS Dune Database Entry Number 0045-031:   ESP_032744_1830   ESP_032955_1830   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.103

4.57

6.42

-3.11

33.9

35.5


  


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