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.

Streamlined Form in Kasei Valles:   ESP_068326_1990   ESP_069474_1990   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.78

283.

-7.8

6.899

45.0

48.4

Inner Channel in Kasei Valles:   ESP_068339_2015   ESP_072111_2015   (Interval in Earth days: 294)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.15

287.

4.31

-13.1

44.6

52.5

Jezero Crater Inlet Valley :   ESP_068162_1990   ESP_067159_1990   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.66

76.6

-7.4

27.38

45.0

48.8

Terrain in Utopia Planitia:   ESP_068121_2145   ESP_072170_2145   (Interval in Earth days: 315)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.10

111.

9.15

22.68

50.2

49.8

Quadruple Exit Breach in Small Fresh Crater:   ESP_068267_1440   ESP_073463_1440   (Interval in Earth days: 405)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.8

99.7

-5.3

7.646

56.9

60.0

Valleys in Crater Northeast of Argyre Region:   ESP_067704_1500   ESP_073784_1500   (Interval in Earth days: 474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

334.

7.13

20.86

44.0

53.7

Gullies with Bright Fans in Noachis Terra:   ESP_067743_1475   ESP_077265_1475   (Interval in Earth days: 742)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.1

351.

3.61

-6.16

46.0

54.6

Lobate Debris Apron on Floor of Barnard Crater:   ESP_067833_1185   ESP_067688_1185   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-61.0

60.2

11.4

-14.6

64.7

63.7

Mounds in Acidalia Planitia:   ESP_068074_2280   ESP_068483_2280   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.47

312.

-7.6

26.38

59.5

53.0

Crater Floor:   ESP_068047_1765   ESP_069182_1765   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.38

336.

-7.5

2.483

42.2

53.5


  


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