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.

Grooves in South Polar Layered Deposits:   ESP_023696_0905   ESP_023539_0895   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.3

144.

26.2

25.54

84.2

81.9

Exposure of South Polar Layered Deposits:   ESP_023795_0925   ESP_023691_0925   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.4

279.

18.1

2.542

84.6

84.6

Possible Hematite and Kieserite in Capri Chasma:   ESP_023753_1660   ESP_024320_1660   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.8

309.

-4.7

8.069

34.3

39.8

Small Floral-Shaped Volcano on a Cerberus Fossa:   ESP_023811_1880   ESP_024378_1880   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.076

162.

7.71

21.56

34.0

33.7

Basal Exposure of South Polar Layered Deposits:   ESP_023773_1025   ESP_023615_1025   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-77.2

129.

25.3

8.468

75.0

73.1

Rugged Banded Material in Crater in Northwest Hellas Planitia:   ESP_023789_1420   ESP_024066_1420   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.7

47.4

21.8

0.082

44.7

50.6

Gullies and Curved Ridges at the Base of Crater Walls:   ESP_023328_1325   ESP_023750_1325   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.3

37.6

0.42

-14.4

45.6

52.9

Colorful Rocks in Terra Sabaea:   ESP_023274_1545   ESP_022773_1545   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.4

66.1

25.7

0

31.4

32.3

Layered Yardangs:   ESP_022774_1865   ESP_023051_1865   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.322

34.6

2.09

-26.7

41.8

40.7

Ultimum Chasma South Polar Layers:   ESP_023456_0990   ESP_041100_0990   (Interval in Earth days: 1375)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.7

155.

7.58

-6.73

73.4

74.7


  


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