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 with Summit Pit Inside 20-Kilometer Diameter Crater:   PSP_006961_2195   PSP_007884_2195   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.02

116.

3.71

-22.2

44.8

43.9

Exposure of High-Latitude Polar Layered Deposits Not Well-Observed:   PSP_005139_0920   PSP_005269_0920   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.7

280.

5.03

18.59

70.9

70.7

Deeply-Incised Channels in Mantled Crater Walls:   PSP_006544_1460   PSP_010750_1460   (Interval in Earth days: 328)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.6

351.

0

-16.0

50.6

71.0

Complex Banded Terrain of Floor of Hellas Basin:   PSP_006278_1410   PSP_010563_1410   (Interval in Earth days: 334)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.7

55.4

0

13.47

49.7

73.5

Exposure of Polar Layered Deposits Not Well Observed:   PSP_005983_0920   ESP_023321_0920   (Interval in Earth days: 1351)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.9

278.

8.62

15.55

83.6

77.5

Look For Unconformity at Base of Interior Layered Deposits:   PSP_006519_1730   PSP_007020_1730   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.74

311.

0

9.783

37.5

42.3

Fresh Unnamed Crater with Ponded Materials and Gullies:   PSP_005985_1455   ESP_013817_1455   (Interval in Earth days: 611)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.0

134.

1.73

24.54

42.1

33.9

Juventae Chasma Layered Kieserite Deposit:   PSP_006915_1760   PSP_007060_1760   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.96

298.

2.79

14.99

40.6

41.3

Syrtis Major Hydrated Crater Floor and Megabreccia in Central Pit:   PSP_005842_1970   ESP_011538_1970   (Interval in Earth days: 444)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.03

71.8

6.01

-18.2

41.4

61.2

Gullies:   PSP_006821_1270   ESP_024121_1270   (Interval in Earth days: 1349)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.6

351.

-0.1

-25.5

68.9

63.9


  


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