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.

Lava Flow in Kasei Valles:   ESP_066848_1985   ESP_067323_1985   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.53

285.

-2.5

-15.5

54.3

50.0

Candidate Recent Impact Site:   ESP_066587_2040   ESP_067062_2040   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.57

206.

6.35

-14.7

60.3

55.8

Gullied Slope:   ESP_066775_1425   ESP_066841_1425   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.2

124.

8.23

-2.84

39.0

39.9

Crater Fill Material:   ESP_066791_2045   ESP_067411_2045   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.10

40.8

-4.5

19.86

58.8

50.1

Subtle Scarp in South Polar Layered Deposits:   ESP_066852_0920   ESP_067078_0920   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.8

221.

18.9

8.195

69.2

73.9

Channel in Terra Sirenum:   ESP_066573_1385   ESP_067668_1385   (Interval in Earth days: 86)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

238.

-8.8

5.627

41.3

49.4

Clay-Rich Stratigraphy South of Coprates Chasma:   ESP_066531_1650   ESP_067626_1650   (Interval in Earth days: 85)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.9

301.

-8.7

5.387

41.4

39.1

Features in Mamers Valles:   ESP_066528_2215   ESP_075391_2215   (Interval in Earth days: 690)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.30

14.3

5.69

-4.18

74.0

73.2

Measure Interaction between Wrinkle Ridge and Paleodune Strata:   ESP_066818_1865   ESP_073993_1865   (Interval in Earth days: 559)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.579

25.5

4.36

22.54

46.9

57.3

Slope Streaks in Arabia Terra:   ESP_066514_2050   ESP_074889_2050   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.59

40.0

-5.9

9.124

62.5

64.9


  


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