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.

Cross-Cutting Channels in Olympica Fossae :   ESP_044735_2050   ESP_044880_2050   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.88

246.

5.00

24.41

41.1

39.7

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

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

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

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

Pits Fissures and Channels East of Olympus Mons :   ESP_044841_1960   ESP_044907_1960   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.86

233.

6.54

-11.9

43.6

45.1

Candidate ExoMars Landing Site in Oxia Palus :   ESP_044811_1985   ESP_062191_1985   (Interval in Earth days: 1354)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.03

335.

-23.

-1.96

45.4

45.4

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

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

Troughs within East Candor Chasma :   ESP_044773_1735   ESP_045406_1735   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.63

292.

13.5

29.45

54.4

51.4


  


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