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.

Light-Toned Unit along Noctis Labyrinthus Plains:   ESP_023425_1700   ESP_024137_1700   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

264.

-5.4

13.39

32.1

35.7

Dune Changes in Green Crater:   ESP_023145_1270   ESP_022855_1270   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.6

351.

20.8

-0.20

45.6

43.7

Tongue-Shaped Flow Feature in Hellas Montes Region:   ESP_023141_1435   ESP_023642_1435   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

101.

-5.7

15.39

37.1

41.8

Dense Cratered Cone Field in Cydonia Region:   ESP_023316_2210   ESP_023606_2210   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.53

353.

1.65

19.46

59.4

54.3

Proposed Landing Site in Mawrth Vallis:   ESP_023488_2050   ESP_023554_2050   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.53

338.

6.73

-14.0

44.9

45.5

Craters in South Polar Layered Material:   ESP_023364_1045   ESP_023469_1045   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.2

148.

-14.

27.20

68.5

68.0

Changes in Intracrater Dunes:   ESP_023186_1765   ESP_023463_1765   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.28

307.

4.33

-23.3

33.1

34.3

Light-Toned Material in Noctis Region Fracture:   ESP_023214_1695   ESP_023926_1695   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

264.

3.07

19.20

31.5

33.2

Light-Toned Phyllosilicates along Plains at Coprates Catena:   ESP_023160_1650   ESP_024017_1650   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

301.

-25.

8.371

33.5

36.4

South Polar Layered Material along Crater Rim:   ESP_023377_1050   ESP_032067_1050   (Interval in Earth days: 677)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.0

146.

7.29

-6.93

67.3

66.2


  


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