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.

Possible Exposures of Polar Layered Deposits in Area Not Well Observed :   ESP_058154_0920   ESP_057968_0920   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.1

84.6

17.3

29.61

70.9

67.6

South Polar Layered Deposits :   ESP_058126_0915   ESP_057702_0915   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.5

150.

17.9

27.49

71.2

65.5

Terrain Sample Near Crater :   ESP_057996_1955   ESP_058207_1955   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.32

20.8

1.07

-13.0

47.1

45.3

Layer Exposure in Eos Chasma :   ESP_058170_1650   ESP_057748_1650   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

313.

6.18

-7.39

29.9

34.2

Western Rim of Rayed Crater in Daedalia Planum :   ESP_058094_1565   ESP_067721_1565   (Interval in Earth days: 750)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

230.

0.94

10.31

30.2

41.6

Exposure of South Polar Layered Deposits :   ESP_058100_0915   ESP_057624_0915   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

122.

19.8

27.08

70.4

65.0

Small Crater :   ESP_058065_2080   ESP_058988_2080   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.57

295.

-0.5

-20.5

55.6

45.1

Channel in Hellas Planitia :   ESP_057928_1420   ESP_058429_1420   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.7

83.9

-4.6

8.373

34.1

36.1

Rayed Crater :   ESP_058182_1720   ESP_076012_1720   (Interval in Earth days: 1389)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.07

345.

0

18.19

32.0

34.1

Candidate Landing Site for 2020 Mission in Northeast Syrtis Major Region :   ESP_057928_1980   ESP_058073_1980   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.88

77.2

-10.

13.69

50.5

47.3


  


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