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.

Look for Change Caused By Mass Wasting Since 2007:   PSP_009648_2650   PSP_010097_2650   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.99

151.

2.16

-12.3

62.3

67.1

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010080_2680   PSP_010856_2720   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.79

209.

-8.2

-6.88

68.7

80.5

Polar Layered Deposits Unconformity:   PSP_010048_2615   PSP_010509_2615   (Interval in Earth days: 36)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.49

49.1

-3.5

16.55

63.8

68.5

Strike Slip Fault in Amazonis Planitia:   PSP_009463_2010   PSP_009608_2010   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.81

200.

-2.4

11.28

47.0

46.3

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

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

Southern Highlands High Thermal Inertia and Spectrally Distinct Materials:   PSP_010326_1560   PSP_010471_1560   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.7

44.9

4.00

18.94

67.2

65.4

Phyllosilicates in Acidalia Region:   PSP_009538_2220   PSP_010039_2220   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.78

309.

0.48

17.37

44.8

46.8

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


  


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