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.

Layers on Hellas Planitia Rim and Proposed Site for Future Exploration:   ESP_023195_1505   ESP_023340_1505   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

66.7

-12.

6.662

35.1

34.9

The 2-Kilometer Diameter Well-Preserved Vaduz Crater:   ESP_023302_2185   ESP_023579_2185   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.23

15.8

1.32

-22.4

57.8

55.3

Crater with Rugged Floor in THEMIS V26860010:   ESP_023396_1490   ESP_024319_1490   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

338.

2.17

16.49

36.5

49.0

Small Mounds in Chryse Planitia:   ESP_023159_1995   ESP_023225_1995   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.36

322.

-2.4

-20.9

45.9

46.3

Polar Layers Exposed on Promethei Lingula Surface:   ESP_023102_0980   ESP_022983_0980   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.0

111.

-8.0

6.991

70.0

67.3

Bedrock Exposed in Rim and Terraces of Crater in Molesworth Crater:   ESP_023126_1520   ESP_023627_1520   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.4

149.

-7.8

15.53

33.7

36.6

Boundary between Ophir and Candor Chasmata:   ESP_023134_1755   ESP_023635_1755   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.67

287.

4.94

27.71

32.9

30.0

Pitted Materials in Bakhuysen Crater:   ESP_020309_1570   ESP_020731_1570   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.8

16.2

8.95

-6.93

57.0

54.4

A Pedestal Crater in Malea Planum:   ESP_022787_1085   ESP_030580_1085   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.3

55.1

-4.6

21.88

56.9

53.9

Wrinkle Ridges in West Meridiani Planum:   ESP_022749_1855   ESP_022960_1855   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.439

357.

5.12

-4.25

41.4

39.6


  


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