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 of Erebus Montes :   ESP_055220_2185   ESP_090048_2185   (Interval in Earth days: 2713)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.23

186.

0

-21.8

57.4

57.1

Junctions between Wide Channels and Narrow Channels :   ESP_055538_1735   ESP_063358_1735   (Interval in Earth days: 609)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.67

151.

-2.0

24.76

53.0

55.7

Linear Vent Structure East of Olympus Mons :   ESP_055403_1975   ESP_059676_1975   (Interval in Earth days: 333)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.36

233.

6.12

-17.6

53.2

36.9

Terrace-Based Well-Preserved Pitted Material of Crater in Kasei Valles :   ESP_055440_2105   ESP_063247_2105   (Interval in Earth days: 608)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.38

302.

-5.1

-25.4

57.9

51.6

Gully Comparison on Northern and Southern Rims of Asimov Crater :   ESP_055570_1330   ESP_064247_1330   (Interval in Earth days: 676)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.6

4.45

-8.2

25.99

65.1

67.5

Cross-Bedding in Layers on Steep Scarp :   ESP_055357_1540   ESP_059986_1540   (Interval in Earth days: 361)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

54.3

7.71

-2.15

57.8

52.5

Crater East of Isidis Region :   ESP_055263_1875   ESP_064204_1875   (Interval in Earth days: 697)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.428

96.2

6.56

-24.0

51.4

58.9

Wrinkle Ridge in Solis Planum :   ESP_055283_1580   ESP_073483_1580   (Interval in Earth days: 1418)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

274.

3.78

-18.8

57.0

59.0

Sinuous Ridges North of Gale Crater :   ESP_055578_1760   ESP_059996_1760   (Interval in Earth days: 344)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.89

137.

20.6

8.802

50.9

39.6

Korolev Crater Layers :   ESP_055260_2530   ESP_055247_2530   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
72.91

163.

7.20

-8.16

74.6

75.5


  


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