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.

Hillslope Morphologies near Holden Crater:   ESP_085705_1550   ESP_085850_1550   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

325.

3.70

23.92

43.7

44.3

Kasei Valles Lava:   ESP_085825_1965   ESP_085614_1965   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.14

285.

4.28

-6.99

39.1

40.5

Hillslope Morphologies in Crater:   ESP_085793_1510   ESP_086294_1510   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

84.7

3.79

-4.91

47.1

55.3

Raised Circular Feature:   ESP_085811_2210   ESP_086246_2210   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.81

305.

-6.0

6.055

51.8

47.1

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_085526_1000   ESP_085513_1000   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-79.7

185.

8.77

-3.25

79.0

79.5

Tributary Channel Surrounded by Complex Craters:   ESP_085414_2060   ESP_085981_2060   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.96

341.

1.97

22.76

46.2

40.5

Eroded Layered Bedrock:   ESP_085567_1555   ESP_085923_1555   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

132.

-6.1

16.95

42.3

45.7

Landform and Dunes in Arabia Terra:   ESP_085625_1910   ESP_085836_1910   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.95

345.

-6.7

2.615

38.8

38.0

Xanthe Dorsa:   ESP_085335_2125   ESP_085480_2125   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.46

337.

-1.4

19.20

51.4

48.4

Northern Terra Cimmeria:   ESP_085541_1740   ESP_086319_1740   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.31

119.

3.84

-8.46

36.1

44.2


  


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