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.

Dune-Ice Topography in Olympia Undae:   ESP_071875_2615   ESP_071545_2615   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.60

229.

-2.1

13.94

65.2

61.1

Potential Channel in Gusev Crater:   ESP_071812_1660   ESP_071891_1660   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.6

175.

-3.7

28.34

63.4

60.8

Classic Barchans:   ESP_071999_2560   ESP_072157_2560   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
75.79

94.0

-8.0

6.782

64.0

65.1

Mesa in Chryse Planitia:   ESP_071806_2045   ESP_071872_2045   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.20

333.

5.73

-17.1

48.7

51.1

North Polar Layered Deposits:   ESP_071809_2685   ESP_071531_2685   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.70

260.

-28.

-20.7

70.4

67.3

Grabens and Ridge South of Melas Chasma:   ESP_071742_1655   ESP_071953_1655   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

287.

-5.0

-21.6

64.1

64.7

Crater in Hydraotes Chaos:   ESP_071635_1810   ESP_072070_1810   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.777

326.

0.01

28.11

56.4

53.8

Athabasca Valles:   ESP_071628_1890   ESP_071483_1890   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.072

155.

8.15

-6.45

52.3

53.6

Layers in Meridiani Planum:   ESP_071647_1865   ESP_071792_1865   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.317

358.

-7.7

6.1

54.6

53.3

ExoMars Landing Site within Oxia Planum:   ESP_071951_1980   ESP_071740_1980   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.68

336.

-2.7

14.17

51.3

49.1


  


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