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.

Toro Crater Floor Deposits:   ESP_017841_1970   ESP_018474_1970   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.31

71.7

-1.4

-21.7

45.8

48.8

Ridges and Flow-Like Forms:   ESP_017734_2075   ESP_071880_2075   (Interval in Earth days: 4219)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.32

111.

-1.2

16.1

42.7

47.9

Layered Deposits in Crater in Western Arabia Terra:   ESP_017936_1890   ESP_060489_1890   (Interval in Earth days: 3315)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.810

-0.9

0.22

-9.82

49.5

41.2

Possible MSL Rover Landing Site in South Eberswalde Crater:   ESP_018056_1555   ESP_018557_1555   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.2

326.

3.37

25.76

69.6

67.3

Repeated Sulfate and Clay Beds in West Gale Crater:   ESP_017786_1745   ESP_017931_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.36

137.

-13.

1.249

57.9

57.2

Impact Induced Landslide in Kamativi Crater:   ESP_017972_1595   ESP_018394_1595   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.1

100.

-6.7

-20.7

67.4

68.0

Eastern Portion of Small Melas Chasma Basin:   ESP_017807_1700   ESP_018875_1700   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.82

283.

-6.2

16.99

60.3

58.1

Sinuous Troughs and Ridges near the Sirenum Fossae:   ESP_017784_1425   ESP_026276_1425   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.2

193.

11.4

-12.5

78.5

77.9

Layered Terrain in Aeolis and Zephyria Regions:   ESP_017825_1760   ESP_018458_1760   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.75

149.

13.9

-9.22

55.2

57.1

Flow Into Breached Crater in Central Elysium Planitia:   ESP_018062_1810   ESP_018484_1810   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.837

160.

-8.0

-21.3

54.3

55.6


  


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