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.

25-Kilometer Diameter Impact Crater of Hellas Basin Floor:   PSP_006766_1355   ESP_020387_1355   (Interval in Earth days: 1062)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.0

51.8

1.99

-12.8

61.4

64.8

Unnamed Well-Preserved Crater in Cimmeria Terra:   PSP_005286_1480   PSP_005576_1480   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.5

140.

-27.

-1.66

36.8

36.4

Bright Layers in Hale Crater Ejecta:   PSP_006756_1465   ESP_023779_1465   (Interval in Earth days: 1327)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

322.

4.57

-11.2

53.6

43.7

Spider Evolution Unfrosted:   PSP_004947_0930   PSP_005104_0930   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.0

98.9

-0.2

16.73

68.1

68.0

Alluvial Fans in Unnamed Crater:   PSP_006528_1585   PSP_007095_1585   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

67.1

0

-14.3

43.3

52.6

Spallanzani Crater - Swirl Patterns in Lower Layers along Northern Margin:   PSP_005565_1220   PSP_005842_1220   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.7

86.3

-5.0

-20.8

52.1

57.2

Gullies Within Central Pit of Bamberg Crater:   PSP_006794_2200   PSP_010301_2200   (Interval in Earth days: 274)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.66

356.

-3.9

21.59

46.9

48.7

Lineated Valley Flow and Dissected Mantle Terrain in Chaotic Region:   PSP_006807_2185   PSP_007097_2185   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.22

2.06

-3.1

14.00

46.0

42.9

Basal Exposure of South Polar Layered Deposits:   PSP_005102_1030   PSP_005155_1030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-76.8

132.

7.05

-13.4

60.2

62.0

Layered Bedrock Exposed in the Central Uplift of Martin Crater:   PSP_005821_1585   ESP_011952_1585   (Interval in Earth days: 477)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

290.

-1.8

21.33

35.0

54.2


  


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