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.

High-Latitude Gullies:   ESP_012803_1185   ESP_012948_1185   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-61.1

106.

-7.2

1.666

52.9

50.6

Floor of Athabasca Valles:   ESP_013526_1895   ESP_013671_1895   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.610

156.

-3.5

12.84

51.2

48.4

Layered Crater Fill Material:   ESP_014017_2085   ESP_022021_2085   (Interval in Earth days: 624)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.99

68.5

0.69

16.01

57.5

64.7

Faulting in South Polar Layered Deposits:   ESP_012762_1070   ESP_013171_1070   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.9

146.

10.3

-12.8

58.0

56.3

Rayed Crater:   ESP_013955_1020   ESP_013968_1020   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-77.8

345.

-6.7

7.228

62.3

61.6

Trough in Phoenicis Lacus:   ESP_013971_1675   ESP_014327_1675   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.2

249.

-2.9

9.647

35.6

32.9

Well-Preserved Crater with Central Peak in Chryse Planitia:   ESP_013810_2085   ESP_022869_2085   (Interval in Earth days: 706)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.43

319.

5.59

-12.7

60.4

56.9

Very Fresh 3 Kilometer Diameter Impact Crater:   ESP_013159_1675   ESP_032121_1675   (Interval in Earth days: 1478)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

98.9

-2.3

-26.9

44.4

34.3

Basal Exposure of South Polar Layered Deposits:   ESP_013791_1070   ESP_014134_1070   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

134.

8.74

-8.76

56.2

60.7

Gullied Crater and Central Uplift:   ESP_013799_1310   ESP_057842_1310   (Interval in Earth days: 3432)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.8

270.

2.07

15.09

41.2

37.9


  


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