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.

Layered Deposits in West Candor Chasma:   ESP_027288_1750   ESP_027644_1750   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.93

282.

-24.

-1.62

58.0

56.1

Survey Layering and Faulting in Layered Deposits in Melas Chasma:   ESP_027367_1690   ESP_027512_1690   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.0

286.

-16.

5.998

60.8

59.1

Crater Exposing Bedrock:   ESP_027323_2145   ESP_053788_2145   (Interval in Earth days: 2062)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.07

40.8

-5.2

5.106

43.9

41.7

Bacolor Crater:   ESP_027030_2135   ESP_027729_2135   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.04

118.

5.21

-8.28

41.8

46.8

Gullies on Central Uplift of Lyot Crater:   ESP_027376_2310   ESP_027297_2310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.44

29.3

10.1

-13.1

45.1

46.6

Vents and Flows in Elysium Planitia Flood Lava:   ESP_027187_1835   ESP_028308_1835   (Interval in Earth days: 88)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.341

157.

-1.8

-13.9

51.9

53.9

Streamlined Features in Olympica Fossae:   ESP_027342_2035   ESP_028463_2035   (Interval in Earth days: 87)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.32

243.

-7.2

-16.5

45.4

53.3

Possible Layered Deposit in Open Basin:   ESP_027256_2125   ESP_060183_2125   (Interval in Earth days: 2565)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.25

68.8

6.35

-2.95

42.6

39.2

Gale Crater:   ESP_027280_1750   ESP_051253_1750   (Interval in Earth days: 1868)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.73

137.

24.2

5.454

54.4

40.6

Dune Migration:   ESP_027343_2610   ESP_027448_2610   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.08

199.

-6.8

13.48

60.5

60.2


  


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