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.

Strange Features in Hellas Basin:   ESP_025160_1445   ESP_042395_1445   (Interval in Earth days: 1343)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.2

58.5

10.2

-13.7

65.2

61.7

Recent 2-Kilometer Impact Crater in Northwest Arabia Region:   ESP_025176_2030   ESP_025242_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.58

334.

6.65

-12.9

38.0

39.9

Changes in Intracrater Dunes:   ESP_025144_1420   ESP_024854_1420   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.7

136.

0.92

-24.0

67.3

64.7

Impact Crater with Central Pit on Floor of Larger Crater:   ESP_025240_1690   ESP_025728_1690   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.6

31.9

2.87

-23.9

50.1

56.6

Fresh Crater:   ESP_024825_1640   ESP_050710_1640   (Interval in Earth days: 2017)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.7

203.

-8.8

3.45

48.7

39.1

Fresh Impact Crater:   ESP_024637_1445   ESP_024927_1445   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.0

300.

-25.

-3.61

59.5

62.5

Flow with Reticulated Ridge Pattern:   ESP_024732_1830   ESP_025655_1830   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.094

219.

2.00

17.91

38.6

45.3

Polygons North of Banded Terrain in Hellas:   ESP_024936_1435   ESP_033494_1435   (Interval in Earth days: 667)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.2

55.4

-3.5

-23.0

63.6

61.5

Mass Movement Feature as Seen in Image CTX Image:   ESP_024669_1680   ESP_025170_1680   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

141.

-3.1

17.74

44.2

49.0

Dunes:   ESP_024737_2005   ESP_024025_2005   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.26

79.1

20.0

1.024

35.6

38.2


  


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