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.

Fractured and Deformed Crater Fill:   ESP_016815_2145   ESP_017883_2145   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.23

1.63

-1.5

10.3

41.0

41.2

Very Recent Small Impact Crater:   ESP_016630_1720   ESP_030291_1720   (Interval in Earth days: 1064)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.08

17.6

-3.5

8.058

52.4

48.4

Deposits on the Floor of Palos Crater:   ESP_016943_1775   ESP_017721_1775   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.67

111.

5.57

-9.88

51.3

55.9

Candidate Landing Site in a Possible Salt Playa:   ESP_016288_1745   ESP_016433_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.64

353.

0.58

17.63

47.4

47.7

Crater:   ESP_016225_2355   ESP_016502_2355   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.29

264.

1.34

-12.8

50.1

49.1

Young Fluvial Valleys on Floor of Lyot Crater:   ESP_016260_2295   ESP_016339_2295   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.00

30.7

0.12

21.90

46.7

44.4

Cliffs in Coprates Chasma:   ESP_016198_1695   ESP_016343_1695   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.4

291.

-1.4

15.71

49.0

49.5

Well-Preserved Large Crater Near Tempe Terra:   ESP_016251_2045   ESP_016396_2045   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.34

280.

1.79

16.28

39.6

38.6

Lobate Landform North of Reull Vallis:   ESP_016047_1410   ESP_020293_1410   (Interval in Earth days: 331)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.6

97.2

4.47

-12.9

64.7

63.9

Bedforms in Crater:   ESP_016122_1425   ESP_016267_1425   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

210.

-7.4

6.812

65.4

66.6


  


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