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.

Junction of Three Polar Troughs:   PSP_010030_2670   PSP_010532_2670   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.74

162.

-8.8

-21.4

67.2

74.3

Exposure of North Polar Basal Unit:   PSP_009945_2645   PSP_010063_2645   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.40

343.

-12.

3.559

65.2

65.5

Western Rim and Ejecta of Very Young 12-Kilometer Diameter Crater:   PSP_009810_2140   PSP_010443_2140   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.45

84.2

7.72

-5.93

45.6

51.8

Pit and Channel on Southwestern Pavonis Mons:   PSP_009923_1785   PSP_010213_1785   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.67

246.

-21.

14.06

58.1

55.7

Distributaries From Athabasca Valles:   PSP_009768_1880   PSP_010045_1880   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.721

154.

7.98

-19.7

51.6

54.3

Potential Paleolake in Crater in Ophir Planum:   PSP_010290_1700   PSP_010435_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

306.

0.86

17.82

60.3

58.8

Well-Preserved Crater on a Steep Slope in Tyrrhena Terra:   PSP_009824_1610   PSP_010246_1610   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

69.0

6.12

-5.57

65.8

65.3

Tooting Crater Southern Ejecta Layer:   PSP_009766_2030   PSP_009832_2030   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.53

207.

2.91

-16.9

47.2

49.2

Volcanic Fissure Vent in Elysium Planitia:   PSP_010269_1900   PSP_010414_1900   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.630

157.

-2.2

14.68

52.9

52.0

Stratigraphy of the North Polar Deposits:   PSP_010198_2645   PSP_010014_2645   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.38

253.

7.14

-7.89

66.8

65.5


  


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