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.

Layers in Floor of Small Crater:   ESP_012911_2165   ESP_013755_2165   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.13

23.1

-0.1

-21.7

74.4

68.5

Mound on Nili Patera Floor:   ESP_013582_1895   ESP_020940_1895   (Interval in Earth days: 574)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.139

67.3

1.63

-17.6

49.9

58.9

Eroded Layers in Northeast Gale Crater with Possible Sulfates:   ESP_013263_1750   ESP_013685_1750   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.72

138.

2.26

-12.3

46.0

41.9

Fractured Lava Dome in Eastern Tharsis Region:   ESP_013904_1970   ESP_013970_1970   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.62

275.

-4.7

-25.2

51.1

51.6

Impact Crater with a Rocky Central Uplift:   ESP_012947_1735   ESP_022441_1735   (Interval in Earth days: 740)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.55

125.

4.88

27.14

48.6

37.0

Rocky Deposit That Appears to Emanate from Warrego Valles Channel:   ESP_012665_1365   ESP_012731_1365   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.1

268.

8.21

-10.4

47.9

48.3

Candidate Landing Site in Terra Sabaea and Tyrrhenna Terra Boundary:   ESP_013925_1580   ESP_014426_1580   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

66.6

0.50

25.72

34.3

32.1

Putative Paleolake:   ESP_013780_1630   ESP_058667_1630   (Interval in Earth days: 3497)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.7

64.7

1.57

-15.2

35.8

31.8

3 Kilometer Diameter Crater on Edge of South Polar Layered Deposits:   ESP_013344_0990   ESP_013463_0990   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.7

112.

-6.3

-22.2

60.8

62.4

Gullies in Dunes:   ESP_014151_1325   ESP_021509_1325   (Interval in Earth days: 573)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.1

19.5

5.65

-10.1

42.1

48.1


  


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