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.

Floor of Mclaughlin Crater:   ESP_033391_2020   ESP_037149_2020   (Interval in Earth days: 293)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.90

337.

1.00

18.02

38.3

51.1

Colorful Crater Rim in Northeast Hellas Planitia:   ESP_033427_1460   ESP_033717_1460   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.5

81.5

3.80

28.82

56.9

59.8

Channels and Central Pit of Terra Cimmeria Crater:   ESP_033556_1435   ESP_042299_1435   (Interval in Earth days: 681)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

158.

21.1

1.451

59.8

60.1

Southern Uzboi Vallis Region:   ESP_033484_1480   ESP_033629_1480   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.7

324.

10.4

23.41

56.2

57.6

Banded Terrain in Northwest Hellas Planitia:   ESP_033441_1440   ESP_033507_1440   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.9

59.2

8.66

-11.1

58.5

60.7

Layered Light-Toned Crater-Filling Material in Northwest Hellas Region:   ESP_033520_1545   ESP_033454_1545   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

62.0

-3.2

18.61

53.2

50.8

Inclined Layers on Crater Floor:   ESP_033518_1405   ESP_033584_1405   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.2

117.

8.25

-11.1

62.1

64.2

Shallow Crater with Fan Connected with Channel in HRSC H2938_0000_Nd3:   ESP_033549_2105   ESP_033839_2105   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.23

345.

-25.

-0.94

42.6

40.0

Candidate New Impact Site:   ESP_033494_1900   ESP_089763_1900   (Interval in Earth days: 4384)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.663

47.0

1.35

10.81

37.9

52.5

Lava-Filled Crater:   ESP_033635_1795   ESP_034268_1795   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.32

158.

8.35

-3.45

41.0

48.0


  


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