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.

Crater Exposing Layers in Icy Deposits:   ESP_089851_2175   ESP_090128_2175   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.92

161.

8.87

-6.46

51.8

56.4

Volcanic Cones in Ceraunius Fossae:   ESP_089650_2050   ESP_089927_2050   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.57

250.

6.19

-14.8

49.8

53.6

Closed Fretted Terrain Valley:   ESP_089724_2185   ESP_089790_2185   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.34

28.0

6.60

-9.01

50.9

52.9

Barchan to Sand Sheet Transition in Central Herschel Crater:   ESP_089892_1655   ESP_090037_1655   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

129.

-3.4

17.28

62.1

60.1

Double Crater:   ESP_089603_2125   ESP_089880_2125   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.26

93.1

-1.8

-20.5

49.9

54.1

Glacier Layering Revealed by Impact Crater on Viscous Flow Features Surface:   ESP_089764_2200   ESP_089487_2200   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.61

17.6

-8.7

10.06

52.8

48.4

Inverted Valley and Rings near Erebus Montes:   ESP_089850_2210   ESP_089217_2210   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.73

187.

7.54

17.77

52.6

45.6

Exposed Layers in Olympia Mensae Icy Outliers:   ESP_089774_2545   ESP_089787_2545   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.13

95.1

-4.3

10.35

64.8

63.9

Northern Gullies on Mesa:   ESP_089662_2300   ESP_090216_2300   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.67

278.

7.68

-17.0

52.5

62.0

Scarp Contact:   ESP_089889_1920   ESP_090166_1920   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.85

207.

1.64

-17.1

53.2

56.1


  


Page 3 of 873 (8,723 images)