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.

Dune Interaction with Residual Polar Ice:   ESP_089075_2590   ESP_088983_2590   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.02

81.5

19.5

4.815

58.2

58.4

Planned ExoMars Landing Site in Oxia Planum:   ESP_088803_1975   ESP_088869_1975   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.32

336.

5.29

-17.1

48.0

49.9

Hydrae Cavus:   ESP_088910_1720   ESP_089055_1720   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.72

298.

-7.2

6.758

60.9

59.9

Crater Deposits:   ESP_088867_2175   ESP_079927_2175   (Interval in Earth days: 696)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.05

28.6

-18.

-8.45

46.7

46.2

Shearing Structures between Viscous Flow Features:   ESP_089078_2200   ESP_089355_2200   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.55

24.6

5.18

-17.0

45.8

49.7

Possible Vent on Volcanic Terrain near Lineated Valley Floor Material:   ESP_089020_2110   ESP_089086_2110   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.47

170.

-7.4

-24.8

46.8

48.8

Flow Entering Fretted Terrain Valley:   ESP_088814_2165   ESP_088590_2165   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.33

31.8

16.4

-18.3

43.3

45.6

Deposits in Ganges Chasma:   ESP_088883_1725   ESP_089094_1725   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.29

314.

5.58

-5.54

59.8

60.4

Terrain Features around Crater in Arabia Terra:   ESP_088875_2215   ESP_088585_2215   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.06

167.

2.85

-12.9

44.9

45.1

Ismenius Cavus Channel and Fan-Looking Feature:   ESP_089052_2140   ESP_089197_2140   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.89

16.6

-6.6

4.435

46.6

46.5


  


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