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.

Field of Cones in the Tartarus Montes:   PSP_008528_2060   PSP_009675_2060   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.80

170.

-7.7

13.02

43.5

45.3

Mounds on Lineated Valley Fill:   PSP_008308_2160   PSP_008888_2160   (Interval in Earth days: 46)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.70

57.0

-6.7

3.944

42.1

42.1

Gullies:   PSP_008477_2150   PSP_008833_2150   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.68

120.

7.49

-8.71

41.0

43.1

Cratered Cones in Isidis Region:   PSP_008887_1985   PSP_009177_1985   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.11

88.2

-12.

9.193

47.0

46.1

Strike-Slip Fault in Amazonis Planitia:   PSP_008540_2020   PSP_009898_2020   (Interval in Earth days: 106)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.90

203.

-6.2

10.50

44.3

47.3

Central Peak of Multi-Ringed Lyot Crater:   PSP_008823_2310   PSP_009245_2310   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.45

29.3

4.70

-11.1

43.3

45.7

Dissected Terraces of an Unnamed Crater:   PSP_008327_1995   PSP_009263_1995   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.27

260.

-6.4

8.129

44.3

46.0

MSL Candidate Landing Site:   PSP_009362_2020   PSP_009507_2020   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.69

78.8

-11.

1.906

47.2

46.5

Rocky Area in Ausonia Cavus:   PSP_009111_1475   ESP_078949_1475   (Interval in Earth days: 5442)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.0

96.6

7.85

-11.8

75.5

75.5

Tightly-Meandering Ridge in Aeolis Planum:   PSP_008621_1750   ESP_016269_1750   (Interval in Earth days: 596)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.93

154.

-8.3

-26.0

56.9

48.9


  


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