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.

Gully Apron on Lobate Debris Apron:   ESP_061595_2250   ESP_061740_2250   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.50

42.4

-7.9

7.224

41.5

40.4

Crater in Arabia Terra:   ESP_061715_2205   ESP_061860_2205   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.19

5.68

7.66

22.78

39.8

38.7

Troughs and Ridges in Chryse Planitia:   ESP_061796_2250   ESP_062086_2250   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.59

314.

0

26.65

41.1

39.4

Crater in Arabia Terra:   ESP_061583_2245   ESP_061728_2245   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.04

10.1

-7.7

7.48

41.4

40.3

Crater in Arabia Terra:   ESP_061636_2130   ESP_061570_2130   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.50

5.11

-8.7

6.895

41.1

39.6

East Ganges Chasma Dunes Interaction:   ESP_061638_1725   ESP_061572_1725   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.50

314.

-1.9

17.63

56.7

55.1

Fresh Exit Breach in Crater:   ESP_061782_1480   ESP_061848_1480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.8

347.

-1.1

-18.3

74.0

75.2

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_061739_1985   ESP_061673_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.39

76.9

-26.

-10.5

46.0

44.3

Topography of Rampart Crater:   ESP_061680_2480   ESP_061601_2480   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.94

233.

8.64

-5.43

48.8

49.9

Sinuous Ridge in Tempe Terra:   ESP_061771_2245   ESP_061916_2245   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.33

276.

3.99

18.81

40.7

39.7


  


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