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.

Depression Near Warrego Valles Uplands:   PSP_005967_1400   ESP_059042_1400   (Interval in Earth days: 4136)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

267.

-3.4

7.221

45.5

45.9

Alluvial Fans in Unnamed Crater:   PSP_006528_1585   PSP_007095_1585   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

67.1

0

-14.3

43.3

52.6

Layered Bedrock Exposed in the Central Uplift of Martin Crater:   PSP_005821_1585   ESP_011952_1585   (Interval in Earth days: 477)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

290.

-1.8

21.33

35.0

54.2

Boundary of Ejecta Layers at Tooting Crater:   PSP_006193_2035   PSP_007116_2035   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.02

208.

0

-13.0

42.2

40.5

Floor of Ares Vallis:   PSP_006940_1900   PSP_007876_1900   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.11

334.

-1.8

20.02

38.4

42.9

Fresh Double-Layered Crater with Possible Ponded Materials:   PSP_006945_2350   PSP_007235_2350   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.57

190.

1.13

12.28

54.1

50.5

Basal Exposure of South Polar Layered Deposits:   PSP_005102_1030   PSP_005155_1030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-76.8

132.

7.05

-13.4

60.2

62.0

Seasonal Monitoring:   PSP_005455_0975   PSP_005547_0975   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.1

225.

1.30

15.98

69.4

69.9

South Polar Layered Deposits Survey:   PSP_005302_0880   PSP_005801_0920   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.7

153.

6.38

18.16

73.1

78.7

Gratteri Crater Continuous Ejecta Blanket:   PSP_005521_1620   ESP_012786_1620   (Interval in Earth days: 566)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.6

200.

3.46

27.99

32.5

44.9


  


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