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.

Candidate Future Landing Site:   ESP_034894_2000   ESP_034960_2000   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.89

342.

5.87

-15.7

42.9

44.9

Lava-Ejecta Interaction in Cerberus Region:   ESP_034664_1865   ESP_034954_1865   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.328

144.

7.04

29.64

46.9

46.6

Secondary Impacts Near Domoni Crater:   ESP_034700_2330   ESP_035333_2330   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
52.54

235.

-4.3

-19.3

44.6

45.5

InSight Mission Candidate Landing Site:   ESP_034783_1850   ESP_034928_1850   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.698

136.

-1.1

12.06

49.0

48.8

Sand Dunes on Crater Floor West of Herschel Crater:   ESP_034744_1650   ESP_034810_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

122.

3.67

-20.3

59.8

61.8

Layered Deposits in West Candor Chasma:   ESP_034804_1740   ESP_035305_1740   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.96

283.

0

19.77

54.9

56.0

Trough with Channels in Elysium Fossae:   ESP_034519_2100   ESP_035020_2100   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.50

140.

4.29

15.4

40.2

40.3

Northern Plains Crater Expansion:   ESP_034727_2310   ESP_034806_2310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.44

218.

-0.1

20.04

43.5

41.6

Possible Terraced Crater in Arcadia Planitia:   ESP_034504_2305   ESP_034636_2305   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.19

186.

5.28

-22.2

43.6

45.6

Candidate Future Landing Site:   ESP_034808_1655   ESP_034874_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.3

175.

1.98

-21.3

60.1

62.0


  


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