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.

Mounds in Western Oxia Colles:   ESP_069802_2005   ESP_069657_2005   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.16

330.

8.76

-7.69

49.3

50.3

Hill Southeast of Jezero Crater:   ESP_069719_1985   ESP_070365_1985   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.19

78.2

-3.7

7.67

50.8

50.0

Recent Crater on Northern Plains:   ESP_069968_2390   ESP_069889_2390   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.81

110.

9.20

-6.73

50.1

51.9

Xanthe Dorsa:   ESP_069763_2235   ESP_070053_2235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.13

313.

-4.8

7.205

48.9

46.9

Channel and Crater in Rahway Valles:   ESP_069755_1910   ESP_070177_1910   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.90

174.

13.4

-18.2

51.7

54.8

Undeveloped Collapse Pit:   ESP_069849_1975   ESP_070060_1975   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.41

127.

7.78

-7.90

50.1

51.5

Fluvial Feature South of Candidate ExoMars Landing Site in Oxia Planum:   ESP_069815_1975   ESP_072017_1975   (Interval in Earth days: 171)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.56

335.

10.7

-21.7

49.9

53.3

Mounds in Southern Jezero Crater:   ESP_069864_1985   ESP_069930_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.13

77.5

12.6

-11.4

49.5

51.5

Rough Terrain in Xanthe Terra:   ESP_069552_1920   ESP_069618_1920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.92

315.

7.8

-6.51

50.7

52.2

Wallrock and Layering Contact in West Candor Chasma:   ESP_069461_1750   ESP_069672_1750   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.03

282.

-8.6

11.65

57.9

58.6


  


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