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.

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

Head of Small Chasma on Edge of North Polar Layered Deposits:   PSP_010079_2625   PSP_010105_2625   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.53

284.

-8.6

4.489

65.1

64.6

Landslide Deposit in Ophir Chasma:   PSP_009750_1760   PSP_009895_1760   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.80

288.

-4.3

12.25

58.0

56.8

Pit and Channel on Southwestern Pavonis Mons:   PSP_009923_1785   PSP_010213_1785   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.67

246.

-21.

14.06

58.1

55.7

Dry Cataracts in Athabasca Valles:   PSP_009702_1900   PSP_009847_1900   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.873

156.

0.40

15.92

51.2

50.3

Cones at Edge of North Polar Layered Deposits:   PSP_009947_2590   PSP_009710_2590   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.66

285.

8.81

-10.7

60.4

59.6

Exposure of Light-Toned Layering along Wallrock in Coprates Chasma:   PSP_009684_1695   PSP_010396_1695   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

290.

-2.2

19.86

61.5

58.8

Possible Flute Casts in Ares Vallis:   PSP_009722_1960   PSP_009867_1960   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.92

329.

2.51

17.22

48.9

48.1

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

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009309_2725   PSP_009589_2675   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.52

327.

-4.7

-14.4

64.2

64.4


  


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