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.

Unnamed Small Rayed Crater in Hesperia Region:   PSP_008135_1520   PSP_008425_1520   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

108.

-4.0

6.037

68.6

70.2

Contact between Two Different Units in Ganges Mensa:   PSP_007666_1725   PSP_008022_1725   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.65

311.

6.47

-5.41

50.4

54.5

Fresh Crater in Tyrrhena Terra:   PSP_007172_1680   PSP_007462_1680   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.7

122.

-7.6

6.154

47.7

50.4

Light-Toned Rock in Central Peak of Alga Crater:   PSP_007573_1555   PSP_007929_1555   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

333.

8.34

-3.28

59.4

64.1

Possible Sulfates in Coprates Chasma:   PSP_007205_1660   ESP_024505_1660   (Interval in Earth days: 1348)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.9

301.

5.58

-16.3

48.4

44.1

Cut Crater in Ganges Chasma:   PSP_008101_1710   ESP_016263_1710   (Interval in Earth days: 636)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.91

314.

-5.3

21.95

55.9

47.3

Naar Crater:   PSP_007046_2030   ESP_025691_2030   (Interval in Earth days: 1453)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.90

317.

3.89

-21.5

39.0

42.0

Finely-Layered Fan Deposit of Possible Subaqueous Origin:   PSP_007087_1700   PSP_007667_1700   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.81

283.

-7.7

22.30

45.8

50.5

Crater with Gullies:   PSP_007652_2230   ESP_024095_2230   (Interval in Earth days: 1282)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.65

328.

-6.0

-27.7

43.8

52.7

Mangala Valles:   PSP_008118_1645   PSP_008408_1645   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.5

210.

4.85

15.67

59.6

61.0


  


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