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.

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

Fresh 5-Kilometer Diameter Crater:   PSP_009532_1640   PSP_010033_1640   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

121.

-7.7

17.88

65.2

62.7

Aprons with Channels in Eos Chasma:   PSP_009327_1665   PSP_009960_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

317.

0

-20.9

63.3

64.2

Unnamed Pristine Crater Near Tempe Terra:   PSP_009526_2045   PSP_010370_2045   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.31

279.

0.18

-20.5

46.1

52.4

Cones at Edge of North Polar Layered Deposits:   PSP_009630_2590   PSP_009670_2590   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.00

299.

8.09

-15.1

58.0

59.9

Small Shield Covering the Noctis Fossae:   PSP_010305_1780   PSP_010661_1780   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.91

256.

-7.0

-0.74

57.3

56.9

Clay-Bearing Unit in the Western Arabia Region:   PSP_009735_1985   PSP_009880_1985   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.19

335.

-7.7

7.217

49.1

48.4


  


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