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.

Well-Preserved 12 Kilometer Impact Crater on East Rim in Isidis Region:   ESP_014016_1945   ESP_022376_1945   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.52

98.4

-8.6

14.23

48.5

51.5

Gullies Observed by MOC:   ESP_012707_1445   ESP_013208_1445   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.4

201.

2.07

23.84

46.6

38.4

Possible Rootless Cones in Hydraotes Chaos:   ESP_013177_1800   ESP_021458_1800   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.053

326.

-4.9

-21.2

49.8

53.9

Dry Falls in the Southern Branch of Kasei Valles:   ESP_013152_1980   ESP_013297_1980   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.90

285.

3.51

15.70

60.2

58.1

Central Structure of a Large Impact Crater:   ESP_013134_1610   ESP_021494_1610   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

62.6

-6.3

14.94

43.1

44.9

Fractured Lava Dome in Eastern Tharsis Region:   ESP_013904_1970   ESP_013970_1970   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.62

275.

-4.7

-25.2

51.1

51.6

Lineated Valley Fill in Nilosyrtis Mensae:   ESP_012883_2135   ESP_013160_2135   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.01

68.2

-3.0

-23.7

72.4

72.3

Gullied 35 Kilometer Diameter Impact Crater in Promethei Terra:   ESP_013660_1475   ESP_013950_1475   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.4

103.

0.16

23.60

36.1

33.5

Channel Cutting Wrinkle Ridge in Phlegra Dorsa:   ESP_012985_2025   ESP_013130_2025   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.00

164.

4.41

19.35

64.2

62.2

Volatiles and Gullies:   ESP_013097_1115   ESP_013585_1115   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-68.4

1.31

2.13

-13.5

53.0

53.2


  


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