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.

Crater Superposed on Mamers Vallis Seen in MOC Image R1802279:   ESP_016366_2125   ESP_016511_2125   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.95

18.7

8.24

20.96

40.0

38.7

Debris Apron Source Area:   ESP_016673_2255   ESP_017741_2255   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.29

276.

-1.2

10.92

43.4

41.3

Central Uplift and Olivine-Rich Ponded Material in Elorza Crater:   ESP_016659_1710   ESP_017081_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.77

304.

10.5

-3.93

52.2

56.4

Crater in Acidalia Planitia:   ESP_016841_2340   ESP_017830_2340   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.72

7.48

5.69

-6.67

45.4

44.9

Rocky Mesas in Western Elysium Planitia:   ESP_016889_1885   ESP_017311_1885   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.145

143.

7.82

-11.8

45.3

48.9

Quasi-Periodic Layering in a Large Crater:   ESP_016776_1810   ESP_016921_1810   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.019

351.

-7.5

9.544

49.0

48.8

Mesa Island in East Acidalia Planitia:   ESP_016301_2250   ESP_016578_2250   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.70

352.

-3.9

-20.7

44.9

45.2

Submerged Rim of Crater and Floor Deposits from Uzboi Vallis:   ESP_016487_1495   ESP_017120_1495   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.0

323.

11.7

-6.42

64.1

71.3

Ejecta of Crater Sectioned by Erosion:   ESP_016896_1710   ESP_025678_1710   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.92

315.

6.04

-5.75

54.6

53.8

Lobate Tongue Terminus in CTX Image:   ESP_016418_2255   ESP_017130_2255   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.06

38.1

-2.1

10.57

44.3

41.3


  


Page 683 of 877 (8,770 images)