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.

West Melas Chasma:   ESP_041991_1715   ESP_042136_1715   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.57

284.

-5.4

10.07

40.8

41.3

Candidate ExoMars Landing Site in Hypanis Valles:   ESP_041937_1920   ESP_042003_1920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.88

314.

16.7

-5.73

35.9

37.9

Channel Containing Streamlined Forms Near Anseris Mons:   ESP_041972_1490   ESP_042117_1490   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.7

86.3

-8.6

5.165

52.1

53.5

Geologic Contact between Fluvial Deposits in Aeolis Dorsa:   ESP_041943_1745   ESP_050303_1745   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.30

154.

-6.0

6.611

39.3

31.5

Banded Flow Terrain on Floor of Hellas Planitia:   ESP_041960_1405   ESP_042039_1405   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.1

54.6

-1.8

27.31

57.1

56.6

Clay-Rich Terrain in Oxia Planum: A Proposed ExoMars Landing Site:   ESP_039154_1985   ESP_065448_1985   (Interval in Earth days: 2049)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.27

335.

-1.2

-20.7

63.6

66.4

Possible Crater in South Polar Layered Deposits:   ESP_041150_0920   ESP_041046_0920   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.7

240.

20.0

6.466

80.0

79.8

Ridges and Light-Toned Outcrops North of Atlantis Chaos:   ESP_041151_1500   ESP_047309_1500   (Interval in Earth days: 480)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

181.

-8.0

2.323

39.6

50.5

Wrinkle Ridge Near Ganges Catena:   ESP_041226_1770   ESP_041160_1770   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.83

290.

-2.8

18.39

34.6

33.0

Layered Crater Wall in Northwest Hellas Planitia:   ESP_041116_1470   ESP_041393_1470   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.6

56.9

-0.3

-23.1

40.2

45.4


  


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