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.

Alluvial Fans in Kasei Valles:   ESP_085363_2035   ESP_085297_2035   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.14

294.

0.51

16.99

45.1

44.7

Northern Terra Cimmeria:   ESP_085541_1740   ESP_086319_1740   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.31

119.

3.84

-8.46

36.1

44.2

North Pole Facing Deposit in Crater:   ESP_085325_2220   ESP_085813_2220   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.70

249.

-2.3

2.947

58.0

51.8

Small Volcanic Cones in Chryse Chaos:   ESP_085362_1885   ESP_085573_1885   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.322

324.

-6.6

4.325

38.7

37.3

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_085526_1000   ESP_085513_1000   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-79.7

185.

8.77

-3.25

79.0

79.5

Ridges near Vernal Crater:   ESP_085651_1840   ESP_086218_1840   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.944

356.

3.12

-8.10

36.7

40.5

Incised Gullies:   ESP_085346_1395   ESP_085491_1395   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.9

46.0

6.28

26.83

46.8

47.7

Tributary Channel Surrounded by Complex Craters:   ESP_085414_2060   ESP_085981_2060   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.96

341.

1.97

22.76

46.2

40.5

Large Isolated Landform at Chryse Planitia Margin:   ESP_085402_1945   ESP_085547_1945   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.22

310.

5.37

29.46

39.9

37.2

Landform and Dunes in Arabia Terra:   ESP_085625_1910   ESP_085836_1910   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.95

345.

-6.7

2.615

38.8

38.0


  


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