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.

Dune Survey:   ESP_092006_1305   ESP_092573_1305   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.9

14.8

6.12

-10.7

49.6

44.1

Candidate Tianwen-3 Landing Region:   ESP_092068_2015   ESP_092134_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.48

111.

21.7

6.118

64.0

64.9

Bedform Change Detection near Mawrth Vallis:   ESP_092152_2045   ESP_092297_2045   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.30

340.

-1.8

12.24

67.1

65.7

Active Gullies:   ESP_092196_1435   ESP_092407_1435   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.1

227.

2.19

-19.1

44.9

43.8

Bedding in Hellas Planitia:   ESP_092163_1395   ESP_092308_1395   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.9

48.8

-3.2

8.148

46.2

43.4

Fresh Crater:   ESP_092207_1670   ESP_092418_1670   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.0

283.

-0.2

-26.7

47.6

47.2

Small Fresh Crater in Syrtis Major Planum:   ESP_091964_1930   ESP_092676_1930   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.05

74.1

-5.1

-19.6

61.3

57.0

Ice-Rich Crater Fill:   ESP_092102_1385   ESP_092168_1385   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

273.

0.24

-14.9

46.9

47.1

Incised Alluvial Fans in Kasei Valles:   ESP_092101_2070   ESP_092035_2070   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.82

293.

-11.

5.252

69.4

68.5

Very Recent Small Crater:   ESP_092211_1630   ESP_092936_1630   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.0

175.

1.60

17.03

46.3

36.7


  


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