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.

Proctor Crater Dune Margin Changes:   ESP_022458_1315   ESP_022603_1315   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.9

29.9

-4.6

9.389

39.7

38.9

Cracks around Spider Features in Ice-Free Manhattan:   ESP_022339_0935   ESP_022259_0935   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.2

99.6

-8.6

6.331

66.3

64.4

Thermally Distinct Terrain West of Slipher Crater:   ESP_022581_1315   ESP_058185_1315   (Interval in Earth days: 2774)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.9

271.

3.16

-19.3

39.3

41.6

Three Odd Circular Features in Western Elysium Planitia:   ESP_022612_1855   ESP_048853_1855   (Interval in Earth days: 2045)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.469

138.

-2.1

14.82

43.5

43.6

Layered Bedrock Exposure on Crater Floor:   ESP_022619_1495   ESP_029832_1495   (Interval in Earth days: 563)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.4

313.

-19.

-2.50

34.9

51.4

Wrinkle Ridges in West Meridiani Planum:   ESP_022657_1775   ESP_023369_1775   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.49

350.

0.52

20.48

38.4

31.2

Libya Montes Layered Deposits and Possible MSL Rover Landing Site:   ESP_022337_1830   ESP_022482_1830   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.786

85.7

2.34

18.75

45.0

42.2

Crater Central Uplift in Arabia Terra:   ESP_022457_2115   ESP_022734_2115   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.94

46.9

-7.3

-28.2

63.9

61.6

Well-Preserved Impact Crater:   ESP_022365_2190   ESP_030989_2190   (Interval in Earth days: 672)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.64

37.1

-3.5

-17.5

70.9

73.5

Arkhangelsky Crater Dunes:   ESP_022605_1390   ESP_023106_1390   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.7

335.

-0.6

16.18

36.3

37.7


  


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