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.

Massif in Reull Vallis:   ESP_024051_1365   ESP_024407_1365   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.2

97.0

7.01

22.35

53.8

59.0

Alluvial Fans and Hanging Valley Morphology in Kasei Valles:   ESP_024215_2030   ESP_024637_2030   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.69

291.

8.75

-2.72

37.8

37.9

Well-Preserved 8 Kilometer Crater:   ESP_024080_1340   ESP_032928_1340   (Interval in Earth days: 690)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.4

25.7

6.66

20.83

55.9

56.0

Prominent Channel Form on Tyrrhena Patera:   ESP_024222_1590   ESP_024723_1590   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.9

107.

-7.9

15.92

43.1

48.9

Fretted Terrains:   ESP_024103_1370   ESP_024248_1370   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.6

118.

-2.2

13.74

54.7

56.3

Banded Landforms in Gullied Kampot Crater:   ESP_024254_1380   ESP_041133_1380   (Interval in Earth days: 1315)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.7

314.

13.2

-3.17

55.8

45.7

Cerberus Fossae Streak and Bedform Changes:   ESP_024075_1930   ESP_024563_1930   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.74

154.

3.78

-23.4

35.2

38.4

Mantle Removal around Gully Fan:   ESP_024027_1345   ESP_024304_1345   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.4

33.9

-5.9

-21.5

55.7

61.3

Proctor Crater Dune Changes:   ESP_024291_1320   ESP_024370_1320   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.6

30.3

-29.

-0.98

63.3

62.9

Candor Chasma Dune Changes:   ESP_024255_1750   ESP_024110_1750   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.79

283.

0.86

-19.4

36.3

36.6


  


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