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.

Dunes Dubbed Newport:   ESP_062824_2560   ESP_062666_2560   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
75.89

314.

5.37

-9.62

58.6

58.2

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_062741_1990   ESP_063387_1990   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.68

77.2

0.54

17.50

47.1

49.4

Possible Equatorial Ice-Rich Material in Schiaparelli Crater:   ESP_062717_1755   ESP_062862_1755   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.47

16.2

-8.8

1.672

57.2

56.5

Northern Mid-Latitude Crater:   ESP_062806_2150   ESP_062740_2150   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.80

100.

-3.6

15.57

45.8

43.6

Flow Deposits in Eastern Ladon Valles Basin:   ESP_062745_1615   ESP_062956_1615   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.2

332.

8.06

-7.02

64.1

64.6

Sinuous Inverted Channel in Large Basin in East Arabia Terra:   ESP_062808_2085   ESP_062874_2085   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.26

45.7

8.60

-12.7

45.0

47.3

Dunes with Furrows:   ESP_062912_2575   ESP_053918_2575   (Interval in Earth days: 701)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.16

75.5

-7.2

7.214

61.0

58.0

Terraced Fan in East Candor Chasma:   ESP_062786_1730   ESP_062997_1730   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.84

292.

-3.2

-17.8

58.1

59.1

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_062662_1990   ESP_062952_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.61

77.2

-29.

-12.5

49.4

49.2

High-Latitude Crater with Patterned Ground:   ESP_062992_2475   ESP_063216_2475   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.07

55.0

-2.5

13.10

56.3

57.9


  


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