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.

Terrain Southeast of Raga Crater :   ESP_028582_1315   ESP_030217_1315   (Interval in Earth days: 128)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.2

242.

7.18

16.21

73.5

48.1

Faulted Layered Deposits in Capen Crater :   ESP_028300_1870   ESP_028366_1870   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.675

13.9

-0.1

-19.6

52.1

53.9

Lava Vent in Impact Crater in Elysium Planitia :   ESP_028387_1790   ESP_028532_1790   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.04

159.

1.53

23.32

53.9

52.1

Crater in Meridiani Planum :   ESP_028525_1790   ESP_034630_1790   (Interval in Earth days: 475)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.71

353.

-6.6

8.99

54.6

50.2

Crater and Adjacent Marte Vallis Flows :   ESP_028452_2005   ESP_028518_2005   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.40

183.

-9.0

-25.1

52.4

54.5

Chaotic Terrain :   ESP_028598_1425   ESP_028888_1425   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.3

164.

3.96

26.14

67.5

62.7

Secondaries of Very Fresh Crater :   ESP_028569_2235   ESP_033817_2235   (Interval in Earth days: 409)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.37

225.

2.51

-9.66

57.3

44.9

Possible Fan in Crater :   ESP_028274_2160   ESP_044388_2160   (Interval in Earth days: 1256)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.86

0.40

-4.9

-23.0

52.1

42.0

Possible Repetitive Bedding in Terra Sirenum Hills :   ESP_028319_1445   ESP_028174_1445   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.3

220.

5.27

-13.6

69.1

71.5

Possible Future Landing Site in Mawrth Vallis :   ESP_028499_2065   ESP_028565_2065   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.98

339.

2.17

-14.7

52.4

54.5


  


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