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 Crater South of Acidalia Planitia :   ESP_059579_2225   ESP_077159_2225   (Interval in Earth days: 1370)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.12

356.

1.21

-18.1

47.4

52.1

Valleys in Crater North of Sacra Sulci :   ESP_059608_2110   ESP_059753_2110   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.93

287.

-7.6

6.675

41.2

39.4

Pitted Mounds in Chryse Planitia :   ESP_059646_2245   ESP_059712_2245   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.09

325.

8.76

-5.79

47.5

47.8

Possible Phyllosilicate-Rich Stratigraphy in Western Mawrth Vallis:   ESP_059738_2050   ESP_060094_2050   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.53

338.

-7.4

5.422

38.1

36.8

Pitted Cones in Coprates Chasma :   ESP_059621_1665   ESP_059977_1665   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

297.

-8.7

5.354

40.0

43.9

Topographic Interactions in Vastitas Borealis :   ESP_059752_2235   ESP_059686_2235   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.21

314.

-7.4

7.36

47.0

46.6

Crater Floor :   ESP_059613_1405   ESP_067407_1405   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

158.

0.61

12.76

55.4

44.0

Crater Floor Deposits :   ESP_059538_2065   ESP_060250_2065   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.17

38.7

-7.1

17.25

39.3

36.2

A Snow Plow Landslide :   ESP_058960_1800   ESP_058894_1800   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.05

341.

-2.6

20.52

31.7

29.8

Gullies on Outer Crater Wall in Nereidum Montes :   ESP_059357_1385   ESP_058935_1385   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

307.

5.31

18.04

52.3

44.5


  


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