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.

Potential Compound Dune in USGS Dune Database 1687-642:   ESP_092317_1155   ESP_092383_1155   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-64.2

168.

0.25

-14.7

52.1

52.5

Streamlined Shapes South of Harmakhis Vallis:   ESP_092425_1385   ESP_092636_1385   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

93.9

2.97

-20.3

42.5

42.2

Triangular Scars on Hillslopes:   ESP_092549_1335   ESP_092325_1335   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.2

308.

3.67

-16.2

42.4

46.3

Holden Crater Sedimentary Fan:   ESP_092456_1525   ESP_092667_1525   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

325.

0.76

-25.0

41.6

41.2

Network of Channels on Rim of Newton Crater:   ESP_092632_1420   ESP_092698_1420   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

200.

-2.6

-25.5

40.1

41.4

Banded or Layered Megabreccia Clasts in Nili Fossae:   ESP_092544_1995   ESP_092610_1995   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.17

76.5

-1.1

-26.7

61.3

62.3

Inverted Channel in Noachis Terra:   ESP_092678_1610   ESP_092177_1610   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.9

22.8

-12.

8.654

41.2

45.8

Alluvial Fan in Kasei Vallis:   ESP_092602_2030   ESP_092681_2030   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.70

292.

-2.3

24.40

63.3

61.0

Possible Eroded Dyke System in Atlantis Chaos:   ESP_092593_1450   ESP_092224_1450   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.7

183.

17.5

-7.74

38.6

45.1

Triangular Scars on Hillslopes:   ESP_092443_1320   ESP_092021_1320   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.7

326.

-24.

-7.02

46.0

50.0


  


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