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.

Characterize Possilbe Rotorcraft Landing Site:   ESP_089283_2205   ESP_089362_2205   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.97

189.

-7.1

19.14

48.3

46.5

Positive Relief Material in Association with Osuga Valles Depression:   ESP_089397_1655   ESP_089542_1655   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.5

323.

-1.7

14.98

63.7

62.2

Dune Interaction with Residual Polar Ice:   ESP_089589_2600   ESP_089470_2600   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.63

97.9

1.02

16.15

64.9

62.5

Deposit in Small Northern Mid-Latitude Crater:   ESP_089527_2115   ESP_089672_2115   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.99

7.69

3.64

17.38

48.9

48.8

Fan-Shaped Deposit in Arcadia Planitia:   ESP_089428_2200   ESP_089494_2200   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.86

188.

6.33

-9.62

48.3

50.2

Possible Vent in Young Lava Flows in Elysium Region:   ESP_089244_2090   ESP_089534_2090   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.68

174.

4.31

28.13

47.1

46.6

Features around Crater in Arabia Terra:   ESP_089592_2190   ESP_089104_2190   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.44

34.3

-16.

10.19

51.6

45.4

Ismenius Cavus Channel:   ESP_089342_2145   ESP_090252_2145   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.01

17.7

5.30

-17.5

47.4

58.3

Skylight Candidate near Elysium Mons:   ESP_089522_2090   ESP_089667_2090   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.91

145.

-3.6

11.04

49.5

49.3

Thermal Anomaly in Young Lava Flows of Elysium Region:   ESP_089284_1970   ESP_089429_1970   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.03

163.

2.69

16.88

49.6

48.9


  


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