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.

Gullies in Light-Toned Rock:   ESP_012795_1395   ESP_013507_1395   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.2

319.

2.74

16.59

45.9

37.2

Ejecta Falling Into Earlier Large Crater:   ESP_013346_1940   ESP_013768_1940   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.86

29.4

6.71

-7.95

55.5

51.3

Well Preserved 20 Kilometer Diameter Impact Crater:   ESP_013684_1455   ESP_020910_1455   (Interval in Earth days: 563)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.0

168.

-2.8

19.71

36.4

51.7

Fretted Terrain-Like Aprons Near Reull Vallis:   ESP_012935_1415   ESP_013212_1415   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

96.9

6.90

-17.4

43.4

41.9

Layered Bedrock in Northeast Hellas Planitia:   ESP_013964_1490   ESP_020267_1490   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.7

82.9

1.84

19.77

34.9

58.9

Exposure of Layers in South Gale Crater with Possible Sulfates:   ESP_014186_1745   ESP_020410_1745   (Interval in Earth days: 485)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.56

138.

8.10

-13.1

35.2

55.9

Channel Carved Into Scarp within Isidis Planitia:   ESP_013186_1945   ESP_013252_1945   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.55

78.4

-2.7

-24.1

58.1

58.9

Western Half of Very Well-Preserved Gullied Crater:   ESP_012807_1505   ESP_012952_1505   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.4

351.

-5.9

9.919

45.8

42.6

Saheki Crater Alluvial Fan Layering Exposed in Eastern Portion of Crater:   ESP_012949_1580   ESP_013226_1580   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

73.0

0.82

-26.3

44.2

42.9

Ares Vallis Wall and Floor Exposures:   ESP_013216_1870   ESP_022143_1870   (Interval in Earth days: 695)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.694

340.

-2.5

20.39

53.0

48.5


  


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