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.

Central Peak of Well-Preserved Unnamed Crater:   PSP_006782_1630   PSP_006927_1630   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.7

331.

-6.1

5.697

45.0

46.2

Layers in Memnonia Sulci:   PSP_006616_1730   ESP_024285_1730   (Interval in Earth days: 1377)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.70

182.

-4.8

22.96

38.8

35.4

Geologic Contact between Wallrock and Light-Toned Layered Deposits:   PSP_005979_1710   PSP_006757_1710   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.80

294.

3.73

-24.0

33.5

42.6

Columnar Jointing Exposed in An Impact Crater in Marte Vallis:   PSP_006774_2020   PSP_007341_2020   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.57

184.

7.5

-9.82

38.5

40.5

Exposure of Polar Layered Deposits in Area Poorly Observed:   PSP_005715_0930   PSP_005951_0930   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.1

19.3

-0.0

13.96

78.8

81.0

Polar Layered Deposit Stratigraphy Near Chasma Australe:   PSP_004801_0950   PSP_005051_0950   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.1

95.0

0.80

15.92

64.9

65.9

Faults in Melas Chasma Wall:   PSP_004977_1695   PSP_005478_1695   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

291.

-3.4

19.19

37.0

31.8

Small Crater Filled By Deltaic Deposits:   PSP_006954_1885   ESP_016250_1885   (Interval in Earth days: 724)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.520

312

-0.3

-27.7

38.5

44.0

Gullies with Bright Color Deposits:   PSP_005082_1365   ESP_012703_1365   (Interval in Earth days: 594)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.0

309.

-0.9

23.99

38.4

46.0

Contact between Polygon and Massif:   PSP_005700_2200   ESP_011818_2200   (Interval in Earth days: 477)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.77

346.

0

-24.3

59.2

72.7


  


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