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.

Marte Vallis Streamlined Landforms:   ESP_014092_1955   ESP_014158_1955   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.46

183.

-6.8

-25.9

48.1

48.6

Gully-Like Features on Dunes in MOC Image R10-03153:   ESP_014067_1150   ESP_021583_1150   (Interval in Earth days: 586)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-64.5

158.

-5.6

20.41

53.4

51.9

Possible Rootless Cones in Hydraotes Chaos:   ESP_013177_1800   ESP_021458_1800   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.053

326.

-4.9

-21.2

49.8

53.9

Geologic Contact North of Arabia Terra:   ESP_014138_2235   ESP_022643_2235   (Interval in Earth days: 662)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.14

3.39

-2.8

24.50

67.8

69.9

Central Structure of a Large Impact Crater:   ESP_013134_1610   ESP_021494_1610   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

62.6

-6.3

14.94

43.1

44.9

Fretted Terrain-Like Aprons Near Reull Vallis:   ESP_012935_1415   ESP_013212_1415   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

96.9

6.90

-17.4

43.4

41.9

Channels and Noachian Crater Fill:   ESP_012709_1445   ESP_013197_1445   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.2

146.

1.58

-27.4

46.6

42.6

Channel Carved Into Scarp within Isidis Planitia:   ESP_013186_1945   ESP_013252_1945   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.55

78.4

-2.7

-24.1

58.1

58.9

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

Faulting in South Polar Layered Deposits:   ESP_012762_1070   ESP_013171_1070   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.9

146.

10.3

-12.8

58.0

56.3


  


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