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.

Xanthe Dorsa:   ESP_069987_2245   ESP_070277_2245   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.03

317.

-7.5

5.319

48.4

46.5

Inlet Valley:   ESP_069653_1990   ESP_071011_1990   (Interval in Earth days: 106)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.77

78.3

9.32

24.07

49.2

48.0

Landforms in Utopia Planitia:   ESP_069837_2120   ESP_070127_2120   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.68

95.0

-8.5

6.367

48.8

47.0

Exposed Cliff of Stratified Deposits in Melas Chasma:   ESP_069751_1670   ESP_070041_1670   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

287.

0.04

17.69

64.1

64.2

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

Pyramus Fossae:   ESP_069627_2295   ESP_070405_2295   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.12

65.3

-9.1

-21.1

50.4

49.1

Layering in Arabia Terra:   ESP_069656_1845   ESP_069313_1845   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.212

-0.4

-4.1

6.566

55.2

51.5

Terraced Crater:   ESP_069768_2265   ESP_070058_2265   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.34

177.

-8.3

2.893

49.7

47.5

Possible Geological Contact Between Two Units:   ESP_069685_1735   ESP_069342_1735   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.56

289.

-3.1

7.599

60.5

56.3

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


  


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