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.

Especially Bright Materials in Candor Chasma:   ESP_011372_1730   ESP_012295_1730   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.78

284.

5.39

20.7

57.4

53.0

Opportunity Imaged by HiRISE:   ESP_011765_1780   ESP_012820_1780   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.14

354.

11.6

-23.9

56.5

53.9

Fresh Impact Crater in Utopia Planitia:   ESP_011287_2165   ESP_011564_2165   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.02

80.5

-2.6

-23.3

62.3

67.7

Crater in Meridiani Planum with Layering:   ESP_011277_1825   ESP_011910_1825   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.221

357.

3.65

-14.2

56.8

59.2

Fan at Valley Mouth:   PSP_010434_1575   ESP_045431_1575   (Interval in Earth days: 2727)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.3

336.

2.50

-20.1

66.0

64.0

Terraced Fan in Aeolis Region:   PSP_009729_1735   ESP_015953_1735   (Interval in Earth days: 485)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.53

141.

5.81

-16.3

58.8

45.4

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009584_2675   PSP_009757_2675   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.31

77.4

-4.6

-21.6

64.0

65.8

Fluvial and Alluvial Features on North Wall of Eos Chasma:   PSP_009894_1665   PSP_010606_1665   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

317.

3.44

21.18

62.6

59.5

Layering in Gigas Sulci:   PSP_009330_1875   ESP_062208_1875   (Interval in Earth days: 4120)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.582

232.

4.36

-6.52

51.2

50.1

Look for Change Due to Mass Wasting on Scarps of Different Slopes:   PSP_009408_2640   PSP_009882_2640   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.00

230.

0.72

16.89

60.3

62.9


  


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