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.

Crater with Exposed Layered Walls Superposed on Ejecta of Larger Crater:   ESP_033067_1580   ESP_059559_1580   (Interval in Earth days: 2064)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

188.

6.07

22.04

43.7

41.7

Possible Terraced Crater in Arcadia Planitia:   ESP_033066_2230   ESP_033501_2230   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.78

209.

-7.0

19.40

50.0

44.4

Large Meander in Sinuous Ridge in Aeolis Region:   ESP_033187_1780   ESP_034321_1780   (Interval in Earth days: 88)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.77

150.

-1.5

7.93

37.7

48.4

Light-Toned Deposits along Coprates Chasma Floor:   ESP_033142_1655   ESP_029028_1655   (Interval in Earth days: 320)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

301.

-5.8

7.091

41.8

55.4

Massif in Northwest Hellas Region:   ESP_033006_1545   ESP_033296_1545   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.0

55.1

2.01

24.62

44.9

47.9

Possible Terraced Crater in Arcadia Planitia:   ESP_033146_2250   ESP_033225_2250   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.40

183.

-0.1

22.61

49.8

47.4

Monitoring Arabia Terra Dune Field:   ESP_032942_1910   ESP_033008_1910   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.73

358.

-1.7

-24.6

36.0

38.1

Complex of Fresh Shallow Valleys:   ESP_033134_1385   ESP_068014_1385   (Interval in Earth days: 2718)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

162.

-0.6

-21.4

57.7

56.8

Gullies:   ESP_032989_1435   ESP_067209_1435   (Interval in Earth days: 2666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

161.

-5.2

6.212

52.1

41.1

2-Kilometer Diameter Crater:   ESP_033096_1445   ESP_033386_1445   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.2

120.

-8.6

14.22

53.4

56.8


  


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