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.

Strike Slip Faults in Amazonis Planitia:   ESP_017045_2015   ESP_018113_2015   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.26

204.

-6.1

8.022

42.8

44.3

Possible Phyllosilicate-Rich Terrain:   ESP_016918_2030   ESP_017986_2030   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.68

71.0

-0.6

12.29

41.6

43.2

East Rim of Well-Preserved Crater on Rim of Larger Crater:   ESP_016971_1610   ESP_017683_1610   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

69.1

-0.5

8.387

61.8

65.0

Possible Chlorites and Prehnite in Northern Plains Crater:   ESP_016933_2310   ESP_017210_2310   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.48

16.5

4.76

-14.3

43.8

44.8

Persbo Crater Ejecta Covered by Lava Flows:   ESP_017060_1890   ESP_017205_1890   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.912

156.

-8.7

5.039

47.2

46.8

Light-Toned Mounds in Acidalia Planitia:   ESP_017132_2250   ESP_017633_2250   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.43

345.

-6.6

5.659

42.7

41.6

Enigmatic Pits in Southern Elysium Planitia:   ESP_017284_1790   ESP_017429_1790   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.07

160.

5.24

19.21

52.3

52.0

Nili Patera:   ESP_016905_1890   ESP_035181_1890   (Interval in Earth days: 1424)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.910

67.6

0

17.66

45.7

47.4

Thermally Distinct Crater in Arcadia Dorsa:   ESP_017097_2340   ESP_017532_2340   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.62

218.

3.64

24.24

44.5

42.0

Central Structure and Layered Bedrock in 25-Kilometer Diameter Crater:   ESP_017002_1535   ESP_017147_1535   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.0

303.

-3.1

10.15

67.4

67.7


  


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