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.

Differential Compaction around a Crater Peak:   ESP_033108_1800   ESP_033253_1800   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.12

146.

6.22

18.28

36.0

36.3

Small Pedestal Crater on Ejecta of Larger Craters:   ESP_032961_1385   ESP_033251_1385   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

206.

-1.0

18.10

54.6

58.4

Pettit Crater Wind Streak and Intracrater Dunes:   ESP_033278_1910   ESP_051027_1910   (Interval in Earth days: 1383)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.80

184.

-6.4

10.56

37.3

34.3

Ridges in Meridiani Planum:   ESP_033206_1800   ESP_033496_1800   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.069

351.

0.89

27.28

37.3

37.8

Tilted Layers in Center of Oudemans Crater:   ESP_033275_1700   ESP_033697_1700   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.92

268.

8.73

-8.81

40.6

47.1

Crater with Trough:   ESP_032965_2315   ESP_033809_2315   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.06

84.6

-2.2

-22.5

56.4

49.7

Floor of East Candor Chasma:   ESP_032918_1720   ESP_032984_1720   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.80

295.

6.17

-19.3

35.9

38.6

Possible Terraced Crater in Arcadia Planitia:   ESP_033079_2280   ESP_033356_2280   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.51

211.

4.74

-16.7

52.2

50.9

Well-Preserved Impact Crater with Steep Slopes:   ESP_032975_1415   ESP_033041_1415   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

183.

-4.1

-24.0

53.1

55.4

Crater on the Northern Plains:   ESP_032904_2300   ESP_033181_2300   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.41

309.

4.58

-17.5

55.6

53.8


  


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