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.

Small Channel South of Mangala Valles:   ESP_074883_1600   ESP_083059_1600   (Interval in Earth days: 637)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.6

209.

6.85

-7.00

42.0

51.1

Extra-Crater Sinuous Ridge:   ESP_074959_1035   ESP_075434_1035   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-76.4

308.

4.75

-17.0

57.4

60.1

Spiders in Interesting Terrain:   ESP_074930_0970   ESP_074904_0970   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.7

26.7

8.19

-7.62

61.4

62.6

South Polar Layered Deposits Impact Site:   ESP_074938_0980   ESP_075268_0980   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.0

175.

-7.9

-21.7

62.0

63.8

Pit on Thick Carbon Dioxide Ice:   ESP_074765_0920   ESP_074474_0920   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

232.

19.2

28.92

64.8

65.8

Variety of Spider Terrain:   ESP_075003_0995   ESP_074911_0995   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.6

189.

8.97

-8.06

59.8

61.0

Martin Crater Central Uplift:   ESP_074946_1585   ESP_075157_1585   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.3

290.

-5.4

-12.7

41.7

39.9

Candidate Lake Deposits Fed by Alluvial Fans:   ESP_074827_1655   ESP_073970_1655   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.5

298.

4.36

-6.62

44.2

54.0

Valleys near Huygens Crater:   ESP_074796_1645   ESP_075007_1645   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.3

64.7

7.34

-6.67

44.1

42.6

Candidate Recent Impact Site:   ESP_074701_1840   ESP_075901_1840   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.830

135.

21.8

7.968

52.4

40.1


  


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