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 Draped over Crater Rim Visible in CTX Image :   ESP_025563_1975   ESP_025207_1975   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.48

209.

15.2

2.131

39.4

38.8

Well-Preserved Crater in Tyrrhena Terra:   ESP_025409_1615   ESP_025686_1615   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.4

98.8

6.51

-17.0

56.6

60.7

Olympus Mons Bedform Change Detections:   ESP_025536_1990   ESP_024824_1990   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.84

227.

-3.2

-23.8

40.5

39.4

Ridges or Flows in Northeast Gale Crater:   ESP_025790_1750   ESP_027135_1750   (Interval in Earth days: 104)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.71

137.

-6.0

3.949

52.2

55.9

Light-Toned Material along Coprates Chasma Wallrock:   ESP_025441_1650   ESP_027973_1650   (Interval in Earth days: 198)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

304.

9.23

-16.1

54.3

61.4

Terra Sabaea Intracrater Bedform Changes Changes:   ESP_025794_1750   ESP_026427_1750   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.07

26.0

18.4

-1.81

50.8

55.5

Channel in Tharsis Region:   ESP_025417_1965   ESP_024916_1965   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.19

235.

17.6

-8.13

38.8

38.5

Branching Ridges:   ESP_025683_1900   ESP_025538_1900   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.786

174.

14.4

-4.30

42.7

43.3

Bedrock Exposed in the Central Uplift of a Unnamed Crater:   ESP_025766_2005   ESP_025700_2005   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.18

69.3

-7.5

11.70

41.5

39.7

Source of Flow Visible in CTX Image P20_008700_1787:   ESP_025697_1805   ESP_037169_1805   (Interval in Earth days: 894)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.572

155.

-6.8

8.034

48.6

54.9


  


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