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.

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 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

Double-Layered Pedestal Crater :   ESP_028307_2305   ESP_033832_2305   (Interval in Earth days: 430)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.26

177.

-4.4

-24.1

56.6

49.4

Impact Crater with Multiple Terraces :   ESP_028376_1660   ESP_028653_1660   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.9

102.

-5.5

-27.2

58.9

59.6

Layered Deposits in West Candor Chasma :   ESP_028211_1735   ESP_028277_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.60

284.

9.17

-11.9

55.3

56.8

Mid-Latitude Crater with Rayed Ejecta :   ESP_028469_2195   ESP_028113_2195   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.38

75.2

8.23

-8.07

54.2

51.1

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

Fresh Crater on Northern Plains :   ESP_028285_2310   ESP_028206_2310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.65

56.3

4.29

-18.7

55.7

56.5

Faulted Plains in Tempe Terra :   ESP_028277_2260   ESP_028409_2260   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.63

275.

8.54

-16.9

53.5

57.4

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


  


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