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.

Inverted Channel East of Arabia Terra:   ESP_068163_1965   ESP_069021_1965   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.13

49.6

-6.4

-20.8

44.3

48.6

Crater in Arabia Terra:   ESP_068257_2180   ESP_069326_2180   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.73

1.86

4.48

-9.08

51.4

48.9

Fresh Crater:   ESP_068112_1615   ESP_068706_1615   (Interval in Earth days: 46)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.1

4.43

-0.2

-8.83

45.6

54.9

Terrain in Utopia Planitia:   ESP_068121_2145   ESP_072170_2145   (Interval in Earth days: 315)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.10

111.

9.15

22.68

50.2

49.8

Chain of Layered Mounds in Chryse Planitia:   ESP_068179_2000   ESP_072663_2000   (Interval in Earth days: 350)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.60

332.

-4.3

21.53

45.1

53.6

Pyramus Fossae:   ESP_068149_2310   ESP_077130_2310   (Interval in Earth days: 700)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.41

66.2

-3.9

-16.6

60.2

57.4

Expanded Secondary Crater Cluster in Arcadia Planitia:   ESP_068250_2220   ESP_069187_2220   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.65

193.

-8.2

0.857

54.4

49.0

Polygonal Cracks in Galilaei Crater:   ESP_068377_1855   ESP_069314_1855   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.364

333.

7.64

-6.05

42.9

52.1

Layer Exposure:   ESP_068405_1720   ESP_067679_1720   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.92

294.

-29.

7.548

48.4

38.8

Jezero Crater Inlet Valley:   ESP_068228_1990   ESP_072000_1990   (Interval in Earth days: 294)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.61

76.5

-7.0

14.20

44.9

49.9


  


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