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.

Topographically-Deflected Ejecta in Chryse Planitia:   PSP_007916_2010   ESP_016078_2010   (Interval in Earth days: 636)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.91

322.

0.50

15.41

41.8

38.0

Craters on an Ice-Rich Debris Apron:   PSP_007832_1385   ESP_060736_1385   (Interval in Earth days: 4123)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

103.

1.98

-19.2

74.9

74.8

Bright Layers in Columbus Crater:   PSP_007710_1500   PSP_008066_1500   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

193.

6.36

-4.46

64.8

69.2

Putative Salt Deposits Detected by THEMIS West of Meridiani Region:   PSP_007770_1770   PSP_008917_1770   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.17

351.

6.87

-11.5

49.0

57.2

Interesting Periglacial Assemblage in Utopia Planitia:   PSP_007384_2225   PSP_009467_2225   (Interval in Earth days: 163)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.22

86.3

-1.0

14.43

44.2

43.1

Geometry of Ramparts for Crater in High Southern Latitudes:   PSP_007800_1365   PSP_009593_1365   (Interval in Earth days: 139)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

258.

-5.1

7.815

76.5

83.0

Russell Crater Dunes:   PSP_007018_1255   PSP_007229_1255   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.2

12.9

3.27

-5.25

73.2

77.0

Santa Fe Crater in Chryse Planitia:   PSP_007244_1995   ESP_016052_1995   (Interval in Earth days: 687)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.19

311.

5.51

19.74

38.9

37.5

Eroded High-Latitude Mantle:   PSP_007159_1405   PSP_007515_1405   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

120.

6.69

-4.42

64.2

69.9

Crater Interior with Light-Toned Rock and Curvilinear Ridge Features:   PSP_007465_1595   ESP_085755_1595   (Interval in Earth days: 6100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.2

42.9

-4.0

-22.9

56.2

44.2


  


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