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.

Alcove in East Candor Chasma Layered Deposits:   ESP_012809_1725   ESP_013310_1725   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.44

293.

-2.1

22.37

50.2

42.7

Possible Blocky Deposit in Melas Chasma:   ESP_013508_1665   ESP_014141_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

289.

6.08

-18.0

39.2

35.6

Crater Fill in Noachis Terra:   ESP_013663_1315   ESP_021601_1315   (Interval in Earth days: 618)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.1

23.9

-1.3

24.37

40.9

44.5

Crater in the Sirenum Fossae Region:   ESP_012918_1450   ESP_013340_1450   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.4

201.

-7.6

-20.0

44.4

40.3

South Polar Layered Deposits Exposed in Bend in Trough Wall:   ESP_013830_0940   ESP_014027_0940   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.7

172.

7.85

26.64

66.5

67.5

Exposure of Thick Layered Deposits in Hebes Chasma:   ESP_013205_1790   ESP_021565_1790   (Interval in Earth days: 651)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.82

283.

-25.

-3.43

50.5

51.4

Eastern Tooting Crater Impact Processes:   ESP_013735_2035   ESP_014157_2035   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.18

207.

6.42

-8.32

57.4

52.6

Dry Falls in the Southern Branch of Kasei Valles:   ESP_013152_1980   ESP_013297_1980   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.90

285.

3.51

15.70

60.2

58.1

Layered Sinuous Ridge in Argyre Planitia:   ESP_012848_1235   ESP_012782_1235   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.2

316.

-7.0

6.567

50.2

50.1

Diverse Layers and Morphologies in North Rim of Hellas Planitia:   ESP_013490_1525   ESP_058166_1530   (Interval in Earth days: 3481)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

64.2

-5.3

5.215

37.6

30.5


  


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