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.

Cones in Isidis Planitia:   ESP_019291_1965   ESP_019924_1965   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.59

82.7

17.0

3.208

48.8

54.0

Pit on the Eastern Flank of Pavonis Mons:   ESP_019351_1795   ESP_019984_1795   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.45

248.

-2.8

-17.6

54.7

56.1

Alluvial Fans in Crater:   ESP_019489_1510   ESP_025291_1510   (Interval in Earth days: 452)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.5

84.0

4.07

-20.3

66.3

63.8

Small Fan in Amenthes Fossae Region:   ESP_019264_1895   ESP_019897_1895   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.201

101.

5.29

-10.3

51.1

54.7

Rim and Ejecta of Very Fresh 7-Kilometer Diameter Crater in Arcadia Region:   ESP_019547_2335   ESP_024848_2335   (Interval in Earth days: 413)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.29

288.

5.88

-21.5

58.3

51.5

Well-Preserved 6-Kilometer Diameter Impact Crater:   ESP_019371_1700   ESP_020571_1700   (Interval in Earth days: 94)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.81

63.1

4.37

-11.4

57.7

55.3

Inverted Channel Floor in CTX Image:   ESP_019249_1745   ESP_019394_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.80

154.

-11.

4.813

57.4

56.0

Lava Vent with Channels:   ESP_019325_1960   ESP_019391_1960   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.69

235.

7.19

-14.6

49.9

52.1

Exhumed Light-Toned Deposit along Coprates Catena Floor:   ESP_019270_1645   ESP_019903_1645   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

301.

4.56

-11.5

60.5

59.0

Exposure of North Polar Layered Deposits:   ESP_019343_2685   ESP_028008_2685   (Interval in Earth days: 675)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.28

50.8

-14.

-24.3

74.8

73.1


  


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