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.

Possible Phyllosilicates in Knobs within Depression on Dichotomy Boundary :   ESP_044995_2165   ESP_052023_2165   (Interval in Earth days: 548)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.32

347.

7.00

27.66

41.0

36.1

Unusual Structures in North Polar Layered Deposits :   ESP_044794_2620   ESP_045308_2620   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.91

60.4

-8.8

5.241

59.7

63.2

Lyot Crater Ejecta :   ESP_044743_2290   ESP_044888_2290   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.48

26.1

-7.7

6.254

43.1

42.6

Candidate ExoMars Landing Site in Oxia Palus :   ESP_044824_1985   ESP_062481_1985   (Interval in Earth days: 1376)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.08

336.

23.1

5.898

41.5

45.8

Channels on Alba Mons :   ESP_044814_2270   ESP_045157_2270   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.47

246.

6.41

-14.1

41.6

45.4

Fractures and Exposed Bedrock in Lyot Crater :   ESP_044756_2300   ESP_045099_2300   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.56

28.7

8.24

-10.8

42.1

45.7

North Polar Layered Deposits 160-Meter Diameter Crater Monitoring :   ESP_044810_2620   ESP_044784_2620   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.84

333.

7.95

-6.74

59.0

59.6

Meridiani Planum :   ESP_044718_1780   ESP_046274_1780   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.19

354.

2.37

19.53

52.6

49.7

Unusual Crater in Amazonis Planitia :   ESP_044855_2090   ESP_044921_2090   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.72

210.

3.03

-12.8

41.0

42.5

Transverse Aeolian Ridges in Scandia Cavi :   ESP_044722_2570   ESP_044405_2570   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.93

226.

2.31

28.96

55.5

52.8


  


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