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.

Contact between Older Shield Volcano and Younger Flows :   ESP_050932_1675   ESP_051077_1675   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

261.

7.50

22.13

40.2

41.0

Hellas Planitia Sand Dune Changes :   ESP_051190_1315   ESP_051111_1315   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.1

61.0

20.5

-6.00

67.7

67.8

Possible Repetitive Bedding in Eastern Medusae Fossae Formation :   ESP_050960_1835   ESP_051105_1835   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.559

216.

-3.8

11.32

35.8

35.8

Meroe Patera Dune Monitoring :   ESP_051084_1875   ESP_050939_1875   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.174

67.7

25.4

12.24

33.7

33.9

Layered Light-Toned Deposits on Floor of Orson Welles Crater :   ESP_050996_1790   ESP_051919_1790   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.19

313.

-4.7

10.12

37.3

45.3

East Ophir Chasma Floor :   ESP_051287_1755   ESP_051999_1755   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.24

289.

-0.1

23.09

41.2

46.7

Channel and Fan Structure of Ceraunius Tholus :   ESP_050945_2050   ESP_051235_2050   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.69

262.

2.86

27.57

37.0

34.5

Streamlined Forms in Lava Channel :   ESP_051104_1940   ESP_051249_1940   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.08

242.

5.71

20.15

35.0

34.4

Pasted-on Material on Crater Ejecta :   ESP_050957_1835   ESP_052025_1835   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.147

297.

-0.6

29.33

35.6

42.4

Candidate ExoMars Landing Site in Oxia Palus :   ESP_051272_1985   ESP_071529_1985   (Interval in Earth days: 1578)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.46

335.

6.24

27.25

35.7

47.6


  


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