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.

Northern Hemisphere Gullies with Layers:   PSP_001528_2210   PSP_002214_2210   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.58

120.

2.07

-20.9

49.9

60.6

Mantled Surface of Ascraeus Mons:   PSP_002196_1920   PSP_002618_1920   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.66

252.

4.69

-8.52

53.6

57.1

Slope Streaks in Acheron Fossae:   PSP_001656_2175   PSP_002632_2175   (Interval in Earth days: 76)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.31

229.

0.77

-25.4

50.8

65.6

Unusual Structure on Crater Rim in West Utopia Planitia:   PSP_001503_2180   PSP_001978_2180   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.53

82.7

0

-14.8

49.4

56.0

Evidence of Multiple Episodes of Gully Formation:   PSP_001684_1410   PSP_002027_1410   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

196.

-6.7

-25.8

74.3

72.5

Oudemans Crater Central Uplift: A Sample of Well-Preserved Layering:   PSP_001602_1700   PSP_002446_1700   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.91

268.

2.60

26.00

58.6

54.6

Eroding Layers in an Impact Crater:   PSP_001503_1645   PSP_002189_1645   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.2

89.6

-0.4

-26.5

61.7

61.1

Exhumed Layers near Nili Fossae:   PSP_002176_2025   PSP_002888_2025   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.23

77.0

5.71

20.84

53.8

59.1

Mojave Crater Floor and Central Uplift:   PSP_002101_1875   PSP_002602_1875   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.517

327.

0

23.88

53.9

53.8

HiRISE Images Mars Pathfinder Site:   PSP_001890_1995   PSP_002391_1995   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.08

326.

-5.8

17.05

52.4

54.4


  


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