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.

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

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

Valleys in Crater South of Miyamoto Crater:   ESP_067347_1755   ESP_066529_1755   (Interval in Earth days: 64)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.36

353.

-10.

5.711

40.0

44.3

Outcrops of Fluvial Deposits in Mesa Flank:   ESP_067605_1760   ESP_066510_1760   (Interval in Earth days: 86)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.80

152.

5.52

-6.48

38.9

45.6

Aonia Terra Dune to Sand Sheet Transition:   ESP_067455_1300   ESP_067323_1300   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.6

293.

-7.3

6.065

51.9

49.2

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

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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