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.

Western Rim and Ejecta of Well-Preserved Impact Crater :   ESP_059458_1610   ESP_059392_1610   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

68.9

-14.

7.85

41.0

38.5

Lava Flows Embaying Impact Crater:   ESP_059452_1540   ESP_076135_1540   (Interval in Earth days: 1300)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

232.

-0.5

-15.5

44.0

37.4

Dense Network of Ridges and Alcoves along Crater Rim :   ESP_059460_1820   ESP_059605_1820   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.028

11.1

-6.9

10.19

34.2

33.8

Well-Preserved Small Impact Crater on Hellas Planitia Floor :   ESP_059261_1380   ESP_067886_1380   (Interval in Earth days: 672)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.7

49.7

-4.4

21.24

51.7

52.2

Weathered Ejecta and Pitted Material Associated with Kontum Crater :   ESP_059397_1480   ESP_051076_1480   (Interval in Earth days: 648)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.8

293.

17.9

1.328

45.8

54.7

Possible Olivine-Rich Crater in Terra Sirenum :   ESP_059322_1515   ESP_076783_1515   (Interval in Earth days: 1361)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.2

182.

-5.0

23.12

43.6

42.7

Gullied Lobate Flow Features :   ESP_059436_1335   ESP_059001_1335   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.3

310.

14.6

-19.1

57.1

51.5

Ancient Bedforms on Gordii Dorsum :   ESP_059268_1895   ESP_059545_1895   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.495

210.

6.39

-21.1

33.0

35.9

Impact Crater with Central Pit :   ESP_059263_1840   ESP_059408_1840   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.060

349.

-8.6

7.628

33.4

32.6

Terminus of Pitted Materials Emanating from Oudemans Crater :   ESP_059411_1735   ESP_059266_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.34

269.

2.11

-14.5

34.4

34.3


  


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