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.

Candidate Future Landing Site:   ESP_034808_1655   ESP_034874_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.3

175.

1.98

-21.3

60.1

62.0

Gully Without Apron:   ESP_034628_2340   ESP_035063_2340   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.73

41.1

-2.0

18.22

45.1

42.5

Dune Change Detection in Juventae Chasma:   ESP_034843_1775   ESP_035054_1775   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.58

298.

2.91

-7.48

53.0

54.8

Fan and Channel Forms in Memnonia Sulci Region:   ESP_034768_1695   ESP_035757_1695   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.5

186.

6.76

-7.65

57.1

61.5

Contact of Medusae Fossae Formation with Flank of Apollinaris Mons:   ESP_034597_1730   ESP_034663_1730   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.92

174.

12.3

-12.5

53.2

55.4

Lava Flow North of Ascraeus Mons:   ESP_034739_1975   ESP_035240_1975   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.37

255.

-1.0

16.11

43.6

44.0

Light-Toned Stratified Materials in Eastern Candor Chasma:   ESP_034896_1725   ESP_036452_1725   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.55

292.

-3.8

11.60

56.7

58.2

Ejecta Flow over and around Pre-Existing Obstacles:   ESP_034690_2175   ESP_035336_2175   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.19

150.

7.52

28.85

40.3

39.0

Layered Rocks of Ophir Mensa:   ESP_034738_1760   ESP_034949_1760   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.81

285.

-3.5

-14.7

53.5

55.5

Domoni Crater Secondaries:   ESP_034845_2305   ESP_035280_2305   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.02

236.

-1.8

22.27

43.3

41.1


  


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