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.

Gullied Crater Wall:   ESP_013207_1365   ESP_031180_1365   (Interval in Earth days: 1401)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.0

232.

3.74

-6.73

41.3

38.2

Very Fresh Small Crater in Hesperia Planum:   ESP_013976_1670   ESP_020279_1670   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

113.

-1.1

19.13

35.3

54.4

Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed:   ESP_013910_0880   ESP_022641_0880   (Interval in Earth days: 680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

216.

8.73

19.64

70.6

70.3

Possible Fan Delta:   ESP_013531_2140   ESP_022036_2140   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.87

17.5

-8.5

21.35

68.7

68.8

Possible Hydrate-Rich Terrain in Ius Chasma:   ESP_013680_1730   ESP_020194_1730   (Interval in Earth days: 508)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.81

274.

-1.6

9.024

40.3

54.7

Exposures of Layered Bedrock Northwest of Hellas Basin:   ESP_012620_1540   ESP_013688_1540   (Interval in Earth days: 84)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.5

55.4

3.80

26.88

47.8

33.4

Crater Wall Carving in MOC Image E0300089:   ESP_013828_1360   ESP_013683_1360   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.4

196.

18.3

8.46

37.6

38.3

Pit Crater:   ESP_013167_1785   ESP_013589_1785   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.32

239.

-7.4

-22.9

49.4

45.4

Phyllosilicate and Possible Chlorite Prehnite Northwest of Hellas Region:   ESP_012765_1535   ESP_013477_1535   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

56.4

7.51

22.87

45.6

35.6

Well-Preserved 8 Kilometer Diameter Crater:   ESP_013650_1230   ESP_013927_1230   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.4

20.2

1.13

-19.3

45.0

47.6


  


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