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.

Abalos Mensa and Abalos Scopuli Region:   ESP_025665_2610   ESP_025718_2610   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.01

280.

7.35

-3.58

60.5

60.6

Wrinkle Ridge Superimposed on Well-Preserved Crater:   ESP_025468_1640   ESP_024835_1640   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.7

288.

-5.8

12.96

56.2

47.5

Reticulate Bedform Change Detection Northwest Ascraeus Mons:   ESP_025667_1960   ESP_026168_1960   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.83

252.

-8.4

18.74

42.3

42.3

Light-Toned Material and Dark Dunes and Gullies:   ESP_025177_2145   ESP_026245_2145   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.12

306.

2.29

29.34

39.6

37.3

Floor of Toro Crater:   ESP_025344_1970   ESP_025067_1970   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.00

71.7

-24.

0.616

41.9

38.4

Daedalia Planum Reticulate Bedform Changes:   ESP_025233_1610   ESP_025088_1610   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

223.

13.9

-2.92

54.3

53.5

Mawrth Region Crater with Possible Sedimentary Features:   ESP_025123_2045   ESP_026811_2045   (Interval in Earth days: 131)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.24

340.

12.4

-19.9

37.4

44.7

Possible Phyllosilicates Northwest of Hellas Region:   ESP_025107_1535   ESP_034232_1535   (Interval in Earth days: 711)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

64.5

7.13

-6.50

58.2

63.5

Slope Streaks in Pettit Crater:   ESP_025287_1920   ESP_025643_1925   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.20

186.

0

14.88

40.5

41.5

Fresh Crater on Northern Plains:   ESP_025366_2305   ESP_025498_2305   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.19

184.

-3.4

-26.3

45.0

46.4


  


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