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.

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

Gullied Slope:   ESP_092065_1385   ESP_092342_1385   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

201.

21.1

-2.61

45.7

43.9

Dune Survey:   ESP_091957_1320   ESP_092313_1320   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.4

273.

-8.5

4.482

51.0

45.2

Interesting Domes and Channels Cutting Ridges:   ESP_092003_1380   ESP_092583_1380   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.7

97.7

-13.

15.44

49.5

40.1


  


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