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.

Sand Dunes in Rabe Crater:   PSP_002824_1355   PSP_003325_1355   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.9

34.5

4.86

26.51

62.9

53.5

Candidate Cavern Entrance Northeast of Arsia Mons:   PSP_003647_1745   PSP_004847_1745   (Interval in Earth days: 94)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.53

241.

-0.5

-16.3

52.3

41.1

Very Fine Layers in Juventae Chasma:   PSP_002590_1765   PSP_002946_1765   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.29

298.

-2.1

6.197

55.9

54.9

Ares Vallis Cataract:   PSP_003538_1885   PSP_004171_1885   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.380

335.

-1.1

-19.6

58.0

56.2

Dark Slope Streak with Streak-Generated Topography:   PSP_003542_2035   PSP_005599_2035   (Interval in Earth days: 160)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.32

223.

7.06

20.76

64.7

47.1

Layers in Galle Crater:   PSP_002655_1280   PSP_003156_1280   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-51.7

329.

2.68

19.66

68.9

59.5

Evros Vallis and Nearby Craters:   PSP_003273_1675   PSP_003695_1675   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.6

13.3

-6.9

-18.2

53.7

51.3

Valleys on the Ejecta Blanket from Cerulli Crater:   PSP_003312_2145   PSP_003378_2145   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.01

21.8

3.34

-13.1

69.5

71.2

Kaiser Crater Dune Field:   PSP_003141_1330   PSP_003629_1330   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.5

19.2

16.3

-7.79

58.1

52.1

Alluvial Fan along a Crater Wall:   PSP_003269_1600   PSP_003691_1600   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.9

123.

-4.2

-15.5

53.2

49.8


  


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