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.

Pedestal Crater Stratigraphy:   ESP_014295_1085   ESP_021956_1085   (Interval in Earth days: 597)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.3

54.2

7.11

28.62

60.8

52.1

Possible Kieserite-Rich Terrain in Hebes Chasma:   ESP_014418_1790   ESP_019864_1790   (Interval in Earth days: 425)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.18

284.

1.76

-16.7

35.6

56.2

Curving End of Chasma Australe Wall:   ESP_014373_0995   ESP_022918_0995   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.3

92.8

5.88

-13.6

69.2

66.4

Multiple Branches of the Cerberus Fossae:   ESP_014383_1910   ESP_022097_1910   (Interval in Earth days: 601)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.66

158.

0.24

-14.4

41.3

53.7

Lineated Valley Fill in Nilosyrtis Region:   ESP_014307_2130   ESP_020188_2130   (Interval in Earth days: 458)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.47

70.8

-0.7

24.40

56.9

58.3

Large Rocky Central Uplift:   ESP_014410_1470   ESP_020423_1470   (Interval in Earth days: 468)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.5

146.

2.49

-12.5

37.2

60.1

Triple Crater Fill and Gullies:   ESP_014263_1435   ESP_014329_1435   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

199.

14.3

-4.42

36.7

38.5

Basal Scarp of South Polar Layered Deposits:   ESP_014424_1070   ESP_022837_1070   (Interval in Earth days: 655)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.7

135.

-1.5

-21.0

64.2

59.4

Gullies and Pasted on Material in Nereidum Montes:   ESP_014391_1365   ESP_050192_1365   (Interval in Earth days: 2790)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.2

310.

-23.

8.653

44.2

47.8

Central Uplift of a Large Crater North of Hellas Planitia:   ESP_014439_1505   ESP_020742_1505   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.2

74.5

5.54

18.53

36.0

53.2


  


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