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.

Distal Rampart of Toconao Crater:   ESP_043125_1590   ESP_043837_1590   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.9

284.

-5.6

19.06

60.0

63.2

Clusters of Small Mesas in Northern Arabia Terra :   ESP_043201_2160   ESP_043834_2160   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.65

1.82

5.82

-4.54

39.4

39.8

Crater with Intersecting Faults in Tempe Terra :   ESP_043283_2220   ESP_043560_2220   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.94

282.

-0.8

-19.2

40.9

41.9

Daedalia Planum Lava Flows :   ESP_043219_1570   ESP_045263_1570   (Interval in Earth days: 159)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.8

238.

-7.5

15.85

62.2

63.0

Hills in Coprates Chasma :   ESP_043177_1655   ESP_042887_1655   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

301.

23.0

-6.26

54.1

53.4

Cratered Lineated Valley Fill :   ESP_043159_2145   ESP_043792_2145   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.31

68.2

9.06

-2.36

39.0

39.6

Fans Layers Channels on Floor of Roddy Crater :   ESP_043216_1575   ESP_044350_1575   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

320.

-6.6

18.53

61.6

65.0

Small Fan in Crater West of Mangala Valles :   ESP_043418_1640   ESP_043563_1640   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

204.

-3.2

14.43

58.6

58.5

Wrinkle Ridge Near Ganges Catena :   ESP_043217_1770   ESP_042716_1770   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.08

290.

2.42

-19.3

49.2

46.8

Terraced and Rounded Crater Rim in West Utopia Planitia:   ESP_043119_2185   ESP_043409_2185   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.38

81.7

-9.4

14.08

41.3

38.7


  


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