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.

Bedrock Exposures in Uzboi Vallis and a Crater Rim:   ESP_013586_1490   ESP_021722_1490   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

323.

-0.0

-28.7

36.4

44.3

Central Structure of an Impact Crater:   ESP_012636_1490   ESP_013137_1490   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

338.

6.49

28.71

47.2

38.5

Lineated Valley Fill in Nilosyrtis Mensae:   ESP_012883_2135   ESP_013160_2135   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.01

68.2

-3.0

-23.7

72.4

72.3

Gullied 35 Kilometer Diameter Impact Crater in Promethei Terra:   ESP_013660_1475   ESP_013950_1475   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.4

103.

0.16

23.60

36.1

33.5

Channel Cutting Wrinkle Ridge in Phlegra Dorsa:   ESP_012985_2025   ESP_013130_2025   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.00

164.

4.41

19.35

64.2

62.2

Volatiles and Gullies:   ESP_013097_1115   ESP_013585_1115   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-68.4

1.31

2.13

-13.5

53.0

53.2

Gullies in Southern Hemisphere Crater:   ESP_013894_1410   ESP_022676_1410   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

195.

-5.6

5.235

37.6

35.2

Eastern Half of Gullied Crater:   ESP_012759_1360   ESP_012904_1360   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.8

222.

7.98

20.17

46.7

43.7

Gully with Bright Deposits:   ESP_013639_1415   ESP_013850_1415   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.1

317.

0.32

-9.19

37.3

37.6

Gullies:   ESP_012734_1265   ESP_012879_1265   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-53.1

188.

-7.8

2.791

50.7

47.9


  


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