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.

Light-Toned Layered Deposits in Valles Marineris :   ESP_043731_1655   ESP_043665_1655   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

298.

7.33

27.69

58.7

57.1

Northern Plains Crater Modification :   ESP_043549_2265   ESP_043615_2265   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.99

220.

-5.7

-18.9

41.7

42.7

Pit Near Elysium Mons :   ESP_043763_2100   ESP_071022_2100   (Interval in Earth days: 2124)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.69

139.

10.5

-3.75

38.7

47.6

Gullied Crater in Tempe Terra :   ESP_043705_2225   ESP_043771_2225   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.98

282.

-5.5

-19.7

40.5

41.7

Smooth and Knobby Terrain in Lyot Crater Ejecta :   ESP_043622_2330   ESP_043754_2330   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
52.55

27.4

-8.9

-29.3

43.9

45.5

Kasei Valles Lava Flow :   ESP_043784_2040   ESP_044760_2040   (Interval in Earth days: 76)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.88

287.

7.53

-25.5

40.0

44.1

Valley Intersecting Crater in Nepenthes Region :   ESP_043685_1895   ESP_044806_1895   (Interval in Earth days: 87)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.196

112.

-4.0

-22.1

45.7

48.5

Well-Preserved Impact Crater in Meridiani Planum :   ESP_043557_1770   ESP_044335_1770   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.99

8.83

-7.2

7.52

51.8

52.9

Mamers Valles Source :   ESP_043794_2210   ESP_044084_2210   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.59

12.4

0.68

25.94

39.7

37.3

Meander in Channel in Cydonia Mensae :   ESP_043623_2160   ESP_051126_2160   (Interval in Earth days: 585)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.86

1.35

1.88

-15.6

39.4

42.2


  


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