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.

Candidate Future Landing Site at Valley North of Jezero Crater:   ESP_032794_1990   ESP_033216_1990   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.03

77.3

7.33

-15.0

38.0

38.9

Sand Patch Southwest of Medusae Fossae:   ESP_032500_1715   ESP_032777_1715   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.24

187.

3.55

-26.3

32.9

37.4

Rocky Massif in Nilosyrtis Mensae Region:   ESP_032781_2090   ESP_032847_2090   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.73

72.1

-5.6

-23.1

43.9

44.7

Incipient Collapse at Cerberus Fossae:   ESP_032791_1895   ESP_040835_1895   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.625

161.

0.32

21.92

35.5

39.2

Eroded Crater:   ESP_032585_1870   ESP_033086_1870   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.825

25.6

-1.1

16.26

35.0

34.5

Lobate Debris Apron:   ESP_032556_1390   ESP_041299_1390   (Interval in Earth days: 681)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.7

103.

5.42

-5.84

47.4

47.7

Impact Crater Exposed By Erosion along Candor Chasma:   ESP_032773_1710   ESP_033195_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.07

294.

1.97

-22.0

35.2

41.6

USGS Dune Database Number 0284-520 Changes:   ESP_032783_1275   ESP_033060_1275   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.0

28.5

-3.4

-25.7

59.8

65.9

Semi-Circular Embayment in Charitum Montes:   ESP_032628_1275   ESP_032773_1275   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.3

300.

-1.9

8.822

57.3

59.2

Fractured Ground in Arabia Terra:   ESP_032704_2155   ESP_032994_2155   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.95

12.2

7.31

26.45

47.7

43.5


  


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