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.

Crater Rim with Possible Columnar Jointing:   ESP_024288_1945   ESP_024710_1945   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.52

98.3

21.7

6.703

34.1

36.4

Alluvial Fans and Hanging Valley Morphology in Kasei Valles:   ESP_024215_2030   ESP_024637_2030   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.69

291.

8.75

-2.72

37.8

37.9

Massif in Reull Vallis:   ESP_024051_1365   ESP_024407_1365   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.2

97.0

7.01

22.35

53.8

59.0

Lava Flow Oozing into a Crater:   ESP_024587_1465   ESP_024877_1465   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

222.

7.47

28.63

55.5

58.7

Mawrth Vallis Stratigraphy Exposed:   ESP_024200_2045   ESP_024055_2045   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.47

341.

1.71

-15.1

39.2

41.2

Field of Transverse Aeolian Ridges in Proctor Crater:   ESP_024449_1320   ESP_024515_1320   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.7

31.0

21.9

4.433

63.1

65.1

Gullies on the South Wall of Dao Vallis near the Confluence with Niger Vallis:   ESP_024315_1435   ESP_031818_1435   (Interval in Earth days: 584)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.1

90.2

-5.0

8.408

53.9

35.4

Colorful Central Peak in an Unnamed Crater:   ESP_023674_1590   ESP_024597_1595   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.5

306.

6.77

24.62

34.8

46.2

Possible Site for Future Exploration in Chryse Region:   ESP_023568_1905   ESP_024201_1905   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.61

316.

3.87

-11.8

36.3

36.1

Exposure of South Polar Layered Deposits:   ESP_023562_0925   ESP_032462_0925   (Interval in Earth days: 693)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.3

180.

7.78

17.44

81.4

81.9


  


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