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.

Ridges in Meridiani Planum :   ESP_050256_1835   ESP_050467_1835   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.322

357.

-7.8

-20.8

33.0

34.5

Scarp in Utopia Planitia :   ESP_050371_2080   ESP_050516_2080   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.74

94.6

-4.7

5.307

42.3

40.4

South Polar Residual Cap :   ESP_050441_0930   ESP_050467_0930   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.7

16.2

17.5

23.99

87.2

87.1

Gully Monitoring :   ESP_050131_1425   ESP_050421_1425   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.3

176.

-7.6

10.70

43.7

47.3

Dark Ridges Over Light-Toned Substrate in Eridania Region :   ESP_050434_1505   ESP_050645_1505   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

181.

-1.4

-12.7

42.8

46.8

Inverted and Altered Light-Toned Terrain in Sirenum Fossae :   ESP_050394_1430   ESP_050684_1430   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.4

193.

9.22

28.20

46.4

50.0

Layered Deposits on Crater Floor :   ESP_050253_1465   ESP_051110_1465   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.3

84.3

-4.5

10.46

42.9

55.8

Terra Sirenum Intra-Crater Dune Changes :   ESP_050117_1165   ESP_050407_1165   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.0

203.

-5.3

5.102

62.6

67.1

Flow Feature in Deuteronilus Mensae:   ESP_050281_2245   ESP_050558_2245   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.03

28.1

8.38

-15.9

53.9

51.9

Impact Crater with Diverse Hydrated Minerals :   ESP_050372_2000   ESP_050794_2000   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.89

65.7

23.5

3.038

35.9

35.8


  


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