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.

Lobate Deposit in Well-Preserved 6-Kilometer Impact Crater:   ESP_064014_2195   ESP_064080_2195   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.39

236.

8.52

-8.51

59.7

62.0

Blocky Terrain in Acidalia Planitia:   ESP_064011_2250   ESP_064090_2250   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.48

319.

-6.3

18.08

62.6

61.8

Crater Cut by Wrinkle Ridge:   ESP_064059_1680   ESP_063914_1680   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.6

94.6

7.89

-7.36

58.0

59.4

Terrain Sample:   ESP_064073_1570   ESP_063928_1570   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.7

73.7

8.23

-6.39

61.1

63.0

Crater in Arabia Terra:   ESP_064049_2245   ESP_063983_2245   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.34

1.85

-7.9

7.096

63.3

61.0

Mid-Latitude Crater with Steep Slopes:   ESP_063846_2205   ESP_070033_2205   (Interval in Earth days: 482)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.01

140.

23.6

3.324

56.0

47.1

Wrinkle Ridge and Channel Intersection Along Huygens Crater Rim:   ESP_064034_1610   ESP_063744_1610   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

56.7

22.8

-4.84

58.9

62.2

Intra-Flow Margins and Flow Edge Margins in Deuteronilus Mensae:   ESP_064022_2275   ESP_064246_2275   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.17

18.0

-4.5

26.36

63.6

64.6

North Polar Residual Ice and Defrosting Dunes:   ESP_063899_2615   ESP_063873_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.63

110.

8.93

-5.93

77.0

77.4

Jezero Crater:   ESP_064165_1985   ESP_072422_1985   (Interval in Earth days: 643)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.87

77.3

0.68

-25.2

57.5

55.9


  


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