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.

Sample of Scalloped Terrain West of Erebus Montes:   ESP_089349_2195   ESP_089072_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.37

187.

-8.3

14.20

48.9

44.9

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

Low Shield Summit Vent in Syria Planum:   ESP_089307_1635   ESP_089452_1635   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.2

260.

-0.1

16.18

64.9

63.4

Curve in Valley in Northern Terra Cimmeria:   ESP_089390_1675   ESP_089535_1675   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.4

154.

-8.8

8.148

63.0

61.6

Layering in Southern Lucus Planum:   ESP_089336_1720   ESP_089481_1720   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.84

187.

4.06

19.82

59.8

58.4

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

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

Channelized Flow in Arcadia Planitia:   ESP_089587_2285   ESP_089455_2285   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.17

169.

-17.

9.076

53.4

49.7

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

Planned ExoMars Landing Ellipse Imaging in Oxia Planum:   ESP_089581_1995   ESP_089291_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.24

335.

3.28

-24.9

50.3

51.5


  


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