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.

Bedform Change Detection near Mawrth Vallis:   ESP_092152_2045   ESP_092297_2045   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.30

340.

-1.8

12.24

67.1

65.7

Candidate Tianwen-3 Landing Region:   ESP_092068_2015   ESP_092134_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.48

111.

21.7

6.118

64.0

64.9

Possible Undercutting along Streamline Feature in Elaver Vallis:   ESP_091995_1705   ESP_092272_1705   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.35

309.

4.49

-12.4

50.6

49.1

Landslides in Valles Marineris:   ESP_089701_1660   ESP_090400_1660   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

303.

0.48

-16.6

62.3

61.2

Probing Below the Surface with Impact Craters:   ESP_089323_2180   ESP_089600_2180   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.68

175.

5.18

-15.4

47.3

51.5

Planned ExoMars Landing Site in Oxia Planum:   ESP_090715_1975   ESP_090781_1975   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.07

336.

4.71

-21.1

58.0

60.7

Capri Chasma Interior with Possible Sulfate-Rich Terrain:   ESP_090782_1670   ESP_091494_1670   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

310.

-2.7

-27.8

58.4

56.6

Crater Floor Outcrop:   ESP_090762_1905   ESP_091487_1905   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.57

134.

-5.1

25.16

58.2

58.3

Fluvial Valley in Arabia Terra:   ESP_090820_2085   ESP_090754_2085   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.33

349.

-19.

3.726

63.7

61.0

Okavango Valles:   ESP_090595_2185   ESP_090516_2185   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.24

8.82

17.2

-4.81

60.9

61.7


  


Page 2 of 881 (8,805 images)