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.

Eroded Crater with Eroded Floor in Hellas Region:   ESP_067435_1385   ESP_076680_1385   (Interval in Earth days: 721)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

116.

-2.8

6.995

46.5

49.9

Collapsed Terrain in Osuga Valles Depression and Part of Relict Channel:   ESP_067678_1650   ESP_068008_1650   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

322.

4.26

-24.2

39.6

45.2

Collapse Terrain South of Orson Welles Crater:   ESP_067388_1785   ESP_074088_1785   (Interval in Earth days: 522)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.41

313.

2.05

15.83

39.7

54.7

Gullied Slope:   ESP_067695_1430   ESP_068104_1430   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.7

222.

-7.1

23.60

48.2

52.8

Hydaspis Chaos:   ESP_067374_1825   ESP_074852_1825   (Interval in Earth days: 582)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.223

335.

-5.0

-17.0

41.3

52.8

Gullies on Mound in Nereidum Montes:   ESP_067335_1355   ESP_074734_1355   (Interval in Earth days: 576)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.3

324.

7.98

-20.5

46.2

45.9

Terrain Sample Northwest of Sytinskaya Crater:   ESP_067520_2235   ESP_068061_2235   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.15

305.

4.04

14.32

62.6

55.5

Feature near South Polar Residual Cap:   ESP_067540_0920   ESP_067565_0920   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.7

182.

13.4

27.64

79.9

79.0

Oyama Crater Rim:   ESP_067664_2045   ESP_067796_2045   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.09

339.

7.76

-5.86

48.5

48.5

Gullied Slope:   ESP_067497_1470   ESP_073920_1470   (Interval in Earth days: 501)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.8

223.

6.55

21.01

42.8

52.4


  


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