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.

West Candor Chasma:   ESP_022567_1735   ESP_022989_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.41

285.

23.0

6.063

35.9

33.2

Possible Light-Toned Layered Unit along Noctis Region Depression:   ESP_022647_1690   ESP_023069_1690   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.6

263.

7.19

-12.3

34.6

33.0

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

Reticulate Bedform Change Detection West of Arsia Mons:   ESP_022648_1735   ESP_022503_1735   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.30

235.

19.6

0.712

35.4

38.3

Lobate Flow Feature in Eastern Hellas:   ESP_022494_1385   ESP_022639_1385   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.1

124.

5.68

20.40

36.0

34.9

Faulted, Layered Deposits in Candor Chasma:   ESP_022343_1735   ESP_022699_1735   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.63

284.

-11.

0.088

40.9

36.1

Reull Vallis:   ESP_022073_1390   ESP_021783_1390   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.5

99.2

2.20

-25.8

38.6

44.1

Possible MSL Rover Landing Site in Crater Floor with Layered Mesa:   ESP_022180_1515   ESP_022246_1515   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.2

56.8

-5.5

-26.2

36.8

37.9

Polar Cap Monitoring Site:   ESP_022145_0940   ESP_022131_0940   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.0

350.

-7.7

6.508

65.3

63.8

Gully Monitoring Site:   ESP_022108_1410   ESP_022385_1410   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

223.

0.66

-26.4

38.0

38.2


  


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