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.

Flow in Tharsis Region:   ESP_088055_2035   ESP_088345_2035   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.45

241.

-21.

-5.64

46.3

45.7

Ridges in Nilosyrtis Mensae:   ESP_088312_2135   ESP_088246_2135   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.36

60.4

2.84

21.93

43.1

41.2

Dark Material in Coprates Chasma:   ESP_087697_1660   ESP_088198_1660   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

298.

0.73

12.47

61.2

62.7

Light-Toned Fractured Material West of Nectaris Montes:   ESP_087710_1655   ESP_087644_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

303.

1.75

21.48

61.6

59.9

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_087725_2165   ESP_087659_2165   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.39

248.

-8.9

6.861

43.1

41.7

Crater with Steep Slopes:   ESP_087605_2480   ESP_088040_2480   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.87

277.

-2.1

12.63

52.1

49.6

4-Kilometer Diameter Rayed Crater:   ESP_087802_1915   ESP_088448_1915   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.13

309.

0.34

12.37

48.0

49.1

North-Pole-Facing Deposit in Crater:   ESP_087778_2285   ESP_088068_2285   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.34

240.

-10.

2.734

44.8

43.5

Isolated Dune Field in Crater Northwest of Syrtis Major Planum:   ESP_087903_2050   ESP_089050_2050   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.85

71.6

-17.

0.922

45.3

47.0

Inverted Drainage Network Deep in Central Valles Marineris:   ESP_087816_1705   ESP_088027_1705   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.41

289.

6.89

-9.49

58.7

60.7


  


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