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.

Margin of South Polar Layered Deposits:   PSP_005025_0975   PSP_005262_0975   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.2

88.9

-4.3

12.29

64.5

66.2

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

Pit with Ridges Associated with Fan in Aeolis Region:   PSP_006525_1795   PSP_007092_1795   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.30

146.

0

-14.7

36.4

42.6

Exposure of Polar Layered Deposits within Southern Residual Cap:   PSP_005029_0930   PSP_005239_0930   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.8

11.6

0.89

15.20

68.5

69.6

Reull Vallis and Valley Cut through Crater:   PSP_006777_1405   PSP_006922_1405   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.3

111.

-3.0

7.022

58.5

60.4

Large Fresh Crater Near Marte Vallis:   PSP_006985_2020   PSP_009912_2020   (Interval in Earth days: 228)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.51

184.

-2.8

-22.3

39.3

50.3

Light-Toned Layering along Plains Southwest of Melas Region:   PSP_005017_1695   PSP_005439_1695   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

279.

-4.5

-21.3

36.6

35.1

Fresh Unnamed Crater with Ponded Pitted Materials:   PSP_006981_2335   PSP_007851_2335   (Interval in Earth days: 68)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.30

288.

-4.7

20.50

53.3

44.8

Tomini Crater Western Ejecta:   PSP_005695_1965   PSP_005985_1965   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.25

125.

-1.0

26.25

42.8

38.2

Lava Falls in Northern Kasei Valles:   PSP_005610_2025   ESP_040659_2025   (Interval in Earth days: 2731)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.00

286.

-5.7

8.888

47.7

50.0


  


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