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_010153_2675   PSP_010603_2675   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.58

25.7

-8.4

-23.4

69.2

76.0

Sapping Features East of Tooting Crater:   PSP_010333_2025   PSP_010689_2025   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.14

208.

-3.9

0.754

50.8

53.1

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

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010163_2675   PSP_010230_2675   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.26

123.

-8.3

-20.4

69.1

70.5

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

Gullies in North Mid-Latitude Crater:   PSP_009744_2305   PSP_010245_2305   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.11

84.3

-0.6

14.78

47.4

50.9

Central Peak of Trinidad Crater:   PSP_009427_1565   ESP_027123_1565   (Interval in Earth days: 1378)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.4

109.

-2.9

-19.4

70.1

69.3

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

Basal Unit and North Polar Layered Deposits in Chasma Boreale Scarp:   PSP_009995_2650   PSP_010128_2650   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.06

0.70

19.4

5.177

65.3

66.6


  


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