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.

Traverse Ramp in Eastern Coprates Chasma:   ESP_080761_1640   ESP_080339_1640   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

306.

2.60

15.19

64.6

64.9

Landscape Evolution in Cydonia Mensae:   ESP_080957_2210   ESP_072926_2210   (Interval in Earth days: 626)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.65

350.

-14.

7.427

54.6

62.2

Dune Interaction with Residual Polar Ice:   ESP_080662_2620   ESP_080688_2620   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.96

107.

-6.9

7.38

65.5

64.9

Crater in Arabia Terra:   ESP_080864_2145   ESP_080363_2145   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.04

7.53

10.5

-7.04

50.7

48.5

Streamlined Landforms Adjacent to Shalbatana Vallis:   ESP_080655_1890   ESP_080721_1890   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.021

317.

5.31

-18.5

53.6

55.7

Acidalia Planitia Impact Crater Exposing Layered Materials:   ESP_080681_2125   ESP_080826_2125   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.22

326.

-7.1

2.814

50.7

51.0

Renaudot Crater Dunes:   ESP_080862_2225   ESP_080928_2225   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.97

62.5

-4.6

-20.0

52.8

54.9

Paleolake Crosscut by Shalbatana Vallis:   ESP_080945_1900   ESP_081433_1900   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.748

319.

6.16

-27.4

54.1

58.8

Crater Ejecta Crosscut by Channels in Aeolis Dorsa:   ESP_080727_1735   ESP_080437_1735   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.32

152.

19.9

-7.28

58.7

61.1

Trough Cutting across Wrinkle Ridge in Labeatis Fossae:   ESP_080788_2095   ESP_086260_2095   (Interval in Earth days: 426)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.03

284.

-5.6

4.56

51.4

42.0


  


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