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.

Small Delta or Fan:   ESP_072815_1725   ESP_072960_1725   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.62

148.

-1.0

12.96

58.5

57.1

Mesa in Utopia Planitia:   ESP_072817_2105   ESP_073107_2105   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.31

89.3

-8.4

14.89

59.1

60.6

Hills in Phlegra Montes:   ESP_073091_2170   ESP_081478_2170   (Interval in Earth days: 654)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.82

163.

27.7

15.69

61.3

57.4

Crater in Arabia Terra:   ESP_072899_2205   ESP_072820_2205   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.26

6.18

17.6

-8.12

60.8

61.8

Possible Inverted Channels on Fan Feature:   ESP_073059_1600   ESP_073204_1600   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.0

327.

7.39

22.17

59.8

57.6

Channel West of Idaeus Fossae:   ESP_072809_2145   ESP_072954_2145   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.10

305.

5.91

16.08

58.8

59.8

Candidate Recent Impact Site:   ESP_073077_2155   ESP_073578_2155   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.08

189.

-4.3

18.95

63.4

67.7

Possible Future Landing Site for Mars Sample Return:   ESP_072567_1990   ESP_072857_1990   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.58

76.9

-11.

11.73

55.6

56.0

A Large New Slump in Eos Chasma:   ESP_071886_1640   ESP_069895_1640   (Interval in Earth days: 155)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.7

315.

-3.4

12.83

64.3

65.6

Dark Patches Formed by Craters:   ESP_071661_1570   ESP_071806_1570   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.8

339.

-7.9

6.204

69.7

68.0


  


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