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.

Sinuous Ridge and Channel Southwest of Capen Crater:   ESP_066990_1850   ESP_067333_1850   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.150

12.7

-2.4

7.947

44.9

41.7

Possible Valleys in Small Central Pit Crater:   ESP_066992_1875   ESP_067467_1875   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.378

317.

1.60

-6.73

45.8

42.9

Dune Encroachment on Nereidum Montes Hillslope:   ESP_067151_1330   ESP_067283_1330   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.6

305.

5.00

-10.6

45.5

48.0

Shallow Channels Entering Collapse Terrain near Orson Welles Crater:   ESP_066979_1780   ESP_073877_1780   (Interval in Earth days: 537)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.90

313.

-5.2

10.09

42.0

55.8

Gully Monitoring and Topography:   ESP_067155_1415   ESP_074132_1415   (Interval in Earth days: 543)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

195.

5.52

26.12

41.5

49.6

Crater Uplift and Ejecta in Tyrrhena Terra:   ESP_067054_1760   ESP_067595_1760   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.93

67.0

3.09

-11.7

40.2

40.2

Inverted Channel Feature:   ESP_067281_1910   ESP_067492_1910   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.84

352.

-7.8

25.81

45.7

41.8

Large New Impact Crater:   ESP_066951_2150   ESP_084385_2150   (Interval in Earth days: 1358)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.67

352.

-1.0

24.80

64.3

64.4

Gullies in Crater in Terra Cimmeria:   ESP_067275_1335   ESP_074041_1335   (Interval in Earth days: 527)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.1

163.

-4.3

6.951

47.2

54.2

Valleys in Crater Northeast of Argyre Region:   ESP_067229_1500   ESP_067361_1500   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

334.

7.83

-10.6

39.0

41.4


  


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