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.

Central Structure of an Impact Crater in Terra Cimmeria:   ESP_013092_1630   ESP_013514_1630   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.8

129.

-6.4

-22.9

44.0

40.3

Very Bright and Sun-Facing Gully Deposits in Hale Crater:   ESP_014008_1430   ESP_014153_1430   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.4

322.

-1.9

12.21

36.7

36.3

Gullies Previously Identified in MOC Image:   ESP_013849_1080   ESP_013981_1080   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.9

354.

-7.6

-22.1

56.8

59.0

Recent Gullies in Well-Preserved Crater:   ESP_013667_1345   ESP_013944_1345   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.2

274.

-4.5

-28.7

40.0

42.2

Light-Toned Layered Material in Trough on North Melas Chasma Wall:   ESP_013495_1720   ESP_014128_1720   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.82

284.

6.24

-18.3

41.5

36.9

Recent Gullies in a Crater in Noachis Terra:   ESP_013222_1410   ESP_013288_1410   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

182.

0.69

-18.8

40.4

41.3

Basal Exposure of South Polar Layered Deposits:   ESP_013145_1070   ESP_013277_1070   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

133.

0.46

-14.5

55.6

56.1

Exposed Strata Near Melas Region Wall:   ESP_013719_1665   ESP_021789_1665   (Interval in Earth days: 629)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

289.

2.48

-8.89

37.2

44.6

Superb Phyllosilicate Mafic Stratigraphy Northwest of Hellas Planitia:   ESP_012923_1540   ESP_013345_1540   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

63.8

-4.0

-17.6

44.3

40.2

Valley in Elysium Region Volcanic Rise:   ESP_013157_2015   ESP_013658_2015   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.49

149.

-6.4

14.55

63.2

56.7


  


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