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.

Gullies:   ESP_032989_1435   ESP_067209_1435   (Interval in Earth days: 2666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

161.

-5.2

6.212

52.1

41.1

Possible Fossil Dunes in Noachis Terra:   ESP_032941_1310   ESP_033020_1310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.9

34.0

-2.6

22.11

60.1

60.2

Candidate New Impact Site Formed between December 2011 and December 2012:   ESP_033093_1605   ESP_059506_1605   (Interval in Earth days: 2058)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.3

198.

5.11

-15.9

42.8

42.1

Ridges in Meridiani Planum:   ESP_033206_1800   ESP_033496_1800   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.069

351.

0.89

27.28

37.3

37.8

Crater with Trough:   ESP_032965_2315   ESP_033809_2315   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.06

84.6

-2.2

-22.5

56.4

49.7

Central Peak of Taxco Crater:   ESP_033273_2010   ESP_042095_2010   (Interval in Earth days: 687)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.64

319.

-3.3

11.76

38.3

37.9

Enigmatic Channels on the Floor of Mangala Valles:   ESP_033053_1640   ESP_033264_1640   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

210.

2.12

-10.2

40.7

44.4

Pedestal Crater in Arcadia Planitia:   ESP_032921_2355   ESP_033145_2355   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.13

204.

-0.0

22.74

59.9

55.7

Well-Preserved Impact Crater with Steep Slopes:   ESP_032975_1415   ESP_033041_1415   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

183.

-4.1

-24.0

53.1

55.4

Floor of East Candor Chasma:   ESP_032918_1720   ESP_032984_1720   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.80

295.

6.17

-19.3

35.9

38.6


  


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