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.

Heart-Shaped Pit in Acheron Catena Seen in MOC M02-01153:   ESP_016977_2165   ESP_017755_2165   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.22

258.

-2.6

-13.7

41.1

42.8

Fracture in Orcus Patera:   ESP_017191_1935   ESP_026896_1935   (Interval in Earth days: 756)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.24

178.

0

13.59

45.3

45.7

Layered Terrain in Zephyria Planum:   ESP_017126_1755   ESP_018115_1755   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.51

155.

4.60

-17.2

53.5

58.1

Possible Al-Clay near Columbus Crater:   ESP_017138_1525   ESP_053585_1520   (Interval in Earth days: 2840)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

191.

-6.9

3.289

69.4

69.5

Well-Preserved Impact Crater:   ESP_017119_1635   ESP_025756_1635   (Interval in Earth days: 673)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.3

347.

2.14

-18.7

61.2

60.0

Crater and Ejecta and Context for MOC Image SP2-47903:   ESP_017046_2080   ESP_017824_2080   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.58

175.

4.05

-7.84

40.8

43.4

Crater in Southeastern Sinus Meridiani:   ESP_017250_1710   ESP_018885_1710   (Interval in Earth days: 128)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.04

10.7

-3.2

15.66

57.6

57.7

Possible Phyllosilicate-Rich Terrain:   ESP_016918_2030   ESP_017986_2030   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.68

71.0

-0.6

12.29

41.6

43.2

East Rim of Well-Preserved Crater on Rim of Larger Crater:   ESP_016971_1610   ESP_017683_1610   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

69.1

-0.5

8.387

61.8

65.0

Gullies with Bright Deposits in Poynting Crater:   ESP_017149_1890   ESP_017294_1890   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.768

246.

-12.

2.349

47.9

47.5


  


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