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 Trinidad Crater:   PSP_009427_1565   ESP_027123_1565   (Interval in Earth days: 1378)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.4

109.

-2.9

-19.4

70.1

69.3

Seasonal Monitoring of Polar Crater with Summer Ice:   PSP_009364_2505   ESP_018766_2505   (Interval in Earth days: 732)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
70.05

13.8

-2.3

-22.2

52.5

58.1

Mounds in Ulysses Fossae:   PSP_009409_1860   PSP_009554_1860   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.804

237.

-7.2

8.646

53.1

52.1

Potential Paleolake in Crater in Ophir Planum:   PSP_010290_1700   PSP_010435_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

306.

0.86

17.82

60.3

58.8

Central Uplift of Hargraves Crater in the Nili Fossae Region:   PSP_009639_2010   PSP_010272_2010   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.73

75.8

-5.4

-21.0

47.8

52.1

Impact Crater on Lava Flow Front in Amazonis Planitia:   PSP_010109_1975   ESP_053848_1975   (Interval in Earth days: 3408)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.14

204.

-6.4

7.576

50.7

44.4

Hydrated Light-Toned Layers on Crater Floor:   PSP_010274_2140   PSP_010696_2140   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.63

17.0

5.05

-8.32

49.3

54.8

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

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

Tooting Crater Southern Ejecta Layer:   PSP_009766_2030   PSP_009832_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.53

207.

2.91

-16.9

47.2

49.2


  


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