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.

Tooting Crater Southern Ejecta Layer:   PSP_009766_2030   PSP_009832_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.53

207.

2.91

-16.9

47.2

49.2

Basal Unit and North Polar Layered Deposits in Chasma Boreale Scarp:   PSP_009995_2650   PSP_010128_2650   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.06

0.70

19.4

5.177

65.3

66.6

Central Uplift of Hargraves Crater in the Nili Fossae Region:   PSP_009639_2010   PSP_010272_2010   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.73

75.8

-5.4

-21.0

47.8

52.1

Flow Lobes in Northern Plains Crater:   PSP_009803_2505   PSP_009935_2505   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
70.28

266.

4.45

-8.78

54.9

57.1

Possible Pingos in Gusev Crater:   PSP_009385_1655   PSP_009886_1655   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

175.

-18.

5.226

65.1

63.0

Hydrated Light-Toned Layers on Crater Floor:   PSP_010274_2140   PSP_010696_2140   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.63

17.0

5.05

-8.32

49.3

54.8

Exposure of North Polar Layered Deposits for Stratigraphic Analysis:   PSP_009471_2670   PSP_009683_2670   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.93

301.

-8.2

-21.8

63.0

65.1

Exposure of Polar Layered Deposits on Ridges and Troughs:   PSP_009969_2630   PSP_010008_2630   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.92

40.8

-1.7

15.24

63.7

63.3

Slope Streaks on Nicholson Crater Mound:   PSP_009371_1800   PSP_009516_1800   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.00

195.

-5.9

9.471

55.9

55.0

Central Peak and Pit with Bedrock Exposures:   PSP_010389_1670   ESP_025751_1670   (Interval in Earth days: 1197)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.9

123.

4.69

-15.0

61.2

57.5


  


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