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.

Fresh Crater with Steep Slopes:   ESP_033867_2350   ESP_034856_2350   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.70

296.

1.32

-8.66

49.4

45.4

Possible Terraced Bullseye-Like Crater in Arcadia Planitia:   ESP_033950_2275   ESP_034240_2275   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.22

193.

-7.3

15.36

45.8

42.6

Fissure near Main Cerberus Fossae:   ESP_033925_1885   ESP_037327_1885   (Interval in Earth days: 266)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.314

160.

2.11

13.86

41.2

53.4

Layering in Gorgonum Chaos:   ESP_033911_1430   ESP_042443_1430   (Interval in Earth days: 665)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.5

188.

-2.9

-21.5

66.6

63.7

Recent Crater:   ESP_033733_2125   ESP_034234_2125   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.16

-0.3

-3.7

21.40

40.9

38.4

Sinuous Ridges with Meanders and Scroll Bars in Aeolis Planum:   ESP_034044_1740   ESP_034189_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.02

153.

0.23

19.2

48.5

48.6

Shallow Crater with Cross-Cutting Valley:   ESP_033880_2200   ESP_034882_2200   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.46

305.

-4.8

23.57

42.8

39.0

Channel in Ceraunius Fossae Region:   ESP_033737_2040   ESP_034370_2040   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.62

250.

8.24

-3.83

38.2

41.0

Lava-Covered Crater in Kasei Valles:   ESP_033709_2040   ESP_033999_2040   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.79

296.

-8.4

21.43

39.6

37.6

Tilted Mesas Near Athabasca Valles:   ESP_033965_1875   ESP_042576_1875   (Interval in Earth days: 671)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.490

148.

0.31

13.81

41.9

39.4


  


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