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.

Light-Toned Blocks in or on Melas Chasma Landslide Deposit:   ESP_022844_1680   ESP_031112_1680   (Interval in Earth days: 644)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.9

285.

2.34

-25.2

32.8

40.5

Clustered Mounds in Hypanis Valles Region:   ESP_023001_1925   ESP_023278_1925   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.31

316.

4.36

-18.6

42.7

41.1

Anastomosing Slope Lineae:   ESP_023020_1900   ESP_023297_1900   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.947

157.

2.53

-20.1

41.1

39.8

The Crazy Floor of the Hellas Basin:   ESP_023234_1460   ESP_024091_1460   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.5

81.5

0.57

28.11

36.3

46.4

Starburst Spiders at a South Polar Cracked and Gullied Site:   ESP_023117_0980   ESP_022998_0980   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.6

66.2

-18.

-2.77

70.6

67.8

Fan-Shaped Deposit in a Valles Marineris Trough:   ESP_022949_1650   ESP_030518_1650   (Interval in Earth days: 590)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.9

299.

-1.6

21.10

32.0

42.9

Light-Toned Material along Valley near Coprates Catena:   ESP_022527_1645   ESP_023028_1645   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.5

300.

1.62

23.37

34.6

29.7

Eastern Half of Iazu Crater:   ESP_022670_1775   ESP_023092_1775   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.69

354.

8.00

-9.77

37.6

34.9

Central Uplift of Impact Crater:   ESP_022454_1470   ESP_022599_1470   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.5

136.

-0.5

16.53

34.4

32.5

Stratigraphy of Kasimov Crater Fill:   ESP_022473_1550   ESP_023119_1550   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.9

337.

-8.5

27.5

34.5

30.2


  


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