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.

Very Bright and Sun-Facing Gully Deposits in Hale Crater:   ESP_014008_1430   ESP_014153_1430   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.4

322.

-1.9

12.21

36.7

36.3

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

Recent Gullies in Well-Preserved Crater:   ESP_013667_1345   ESP_013944_1345   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.2

274.

-4.5

-28.7

40.0

42.2

Crater between Branches of Athabasca Valles:   ESP_013460_1900   ESP_013737_1900   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.648

157.

4.42

-23.9

51.5

50.0

Central Structure of Verlaine Crater:   ESP_013213_1705   ESP_013635_1705   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.25

64.1

-1.2

-15.7

44.8

40.8

Nili Fossae-NE Syrtis Phyllosilicate-Sulfate Stratigraphy:   ESP_013041_1975   ESP_030025_1975   (Interval in Earth days: 1324)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.42

76.9

-3.2

12.81

61.2

60.4

Possible Fan Delta:   ESP_013531_2140   ESP_022036_2140   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.87

17.5

-8.5

21.35

68.7

68.8

Light-Toned Outcrop in Hummock of Iani Chaos:   ESP_013717_1790   ESP_013862_1790   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.05

342.

5.13

18.19

42.1

39.5

Lobate Features in the Charitum Montes:   ESP_013165_1275   ESP_013244_1275   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-51.9

301.

-4.0

20.40

45.0

42.6

Well Preserved 20 Kilometer Diameter Impact Crater:   ESP_013684_1455   ESP_020910_1455   (Interval in Earth days: 563)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.0

168.

-2.8

19.71

36.4

51.7


  


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