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.

Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin:   PSP_007377_1700   PSP_008379_1700   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.82

283.

5.56

-6.99

48.4

58.5

Granicus Valles Subchannel Breakout From Main Channel:   PSP_007725_2075   PSP_007936_2075   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.11

136.

7.86

-8.35

40.0

41.8

Complex Layered Deposits in Tithonium Chasma:   PSP_007918_1755   PSP_008274_1755   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.64

270.

6.16

-5.59

51.1

54.6

Possible Sulfates in Ius Chasma:   PSP_007509_1720   ESP_050839_1720   (Interval in Earth days: 3376)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.70

279.

-2.3

13.43

49.3

36.5

Dune Field in Impact Crater Near Cerberus Fossae:   PSP_008159_1885   PSP_008449_1885   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.564

169.

-6.9

2.406

47.4

48.2

Layering in East Coprates Chasma Wall:   PSP_007864_1655   PSP_007508_1655   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

307.

-8.1

4.599

57.2

52.4

Light-Toned Tilted Layering in Central Peak of Oudemans Crater:   PSP_007694_1700   ESP_027882_1700   (Interval in Earth days: 1574)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.92

268.

1.09

-17.4

52.3

59.3

Polygonal Fractures in Utopia Planitia:   PSP_008069_2195   PSP_008504_2195   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.95

102.

-5.9

5.466

42.2

41.3

Ganges Mensa:   PSP_007521_1725   PSP_007877_1725   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.23

311.

7.88

-4.81

48.5

53.0

Light-Toned Outcrops Exhumed From Dark Material in Arabia Terra:   PSP_008139_1905   PSP_009576_1905   (Interval in Earth days: 112)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.54

355.

-7.9

17.40

46.6

49.4


  


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