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.

Low Aspect Ratio Layered Ejecta Crater :   ESP_045225_1810   ESP_080686_1810   (Interval in Earth days: 2763)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.021

194.

6.18

-14.8

49.8

58.2

Southeastern Ejecta Feature of Noord Crater :   ESP_045048_1600   ESP_045470_1600   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.6

348.

-4.0

8.162

63.1

60.3

Herschel Crater Dunes :   ESP_045333_1655   ESP_045478_1655   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

128.

1.55

23.75

58.1

55.9

Exposed Bedrock in Western Central Uplift of 10-Kilometer Diameter Crater :   ESP_045287_1615   ESP_045221_1615   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.3

305.

-7.6

11.12

61.4

60.5

Possible Carbonate Deposit in Crater Floor at Mawrth Vallis :   ESP_045325_2045   ESP_044692_2045   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.05

342.

1.64

-12.8

43.2

42.8

High-Latitude Exposure of North Polar Layered Deposits :   ESP_045251_2720   ESP_045223_2720   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.16

87.4

-8.4

-18.6

69.0

70.1

Slope Monitoring :   ESP_045396_2045   ESP_046464_2045   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.22

203.

2.76

13.00

43.3

51.8

North Polar Gypsum Dunes :   ESP_045263_2605   ESP_045500_2605   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.40

213.

4.05

18.68

61.7

63.6

Candidate Landing Site for 2020 Mission in Nili Fossae :   ESP_045137_2015   ESP_045071_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.03

74.2

-1.3

15.66

43.3

41.7

Eroded Bedrock in Terra Sirenum :   ESP_045238_1525   ESP_051976_1525   (Interval in Earth days: 525)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

203.

-2.0

-16.4

67.0

64.2


  


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