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.

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084894_1050   ESP_084762_1050   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.0

156.

-0.7

14.00

65.3

62.6

Small Terraced Crater:   ESP_084549_2150   ESP_084628_2150   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.88

198.

-7.5

14.22

64.1

61.8

Channel with Streamlined Forms in Northeast Hellas Planitia:   ESP_084725_1445   ESP_085635_1445   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.1

80.2

0

-22.7

37.9

50.3

Well-Preserved 2 to 3-Kilometer Superposed Impact Crater:   ESP_084530_1520   ESP_084741_1520   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

4.19

6.05

-21.1

34.9

37.3

Cratered Cones in Amazonis Planitia:   ESP_084866_2075   ESP_085011_2075   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.42

182.

-3.2

6.99

53.9

51.4

Tectonics on Northern Coprates Chasma Wall:   ESP_084506_1670   ESP_084585_1670   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.6

299.

-16.

14.14

37.5

34.7

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084841_0965   ESP_084815_0965   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-83.2

171.

8.58

-6.10

70.6

71.2

Terraced Impact Crater on Lobate Debris Apron:   ESP_084759_1385   ESP_084825_1385   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

232.

2.14

-19.6

40.6

42.6

Small Fresh Crater:   ESP_084536_1160   ESP_085195_1160   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.8

208.

-2.9

29.34

52.6

59.7

Ridge in Lava Flow:   ESP_084774_2075   ESP_084550_2075   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.39

173.

5.97

-20.2

54.6

59.1


  


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