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 Candor Chasma:   ESP_017675_1760   ESP_017886_1760   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.13

285.

5.36

-4.03

55.6

56.7

Valley Crossing Mare-Type Ridge in Solis Planum:   ESP_017425_1565   ESP_017926_1565   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.1

274.

-3.0

16.24

67.9

68.1

Degrading Craters on Northern Plains:   ESP_017308_2315   ESP_017598_2315   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.90

220.

-9.0

6.936

44.2

42.7

Central Uplift of a Northern Plains Impact Crater:   ESP_017453_2315   ESP_024969_2315   (Interval in Earth days: 586)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51

220.

-6.6

9.417

43.9

46.9

Layering Exposed in Crater Walls:   ESP_017382_1825   ESP_028063_1825   (Interval in Earth days: 833)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.570

5.14

0.74

-11.5

51.1

53.6

Deflected Ejecta of Arabia Region Crater:   ESP_017356_2175   ESP_024872_2175   (Interval in Earth days: 586)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.02

350.

0

20.49

41.2

39.9

Terraced Pedestal Crater in CTX Image:   ESP_017497_2325   ESP_017774_2325   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
52.23

97.6

3.87

-14.3

43.3

45.0

Well-Preserved 6-Kilometer Diameter Impact Crater:   ESP_017334_2300   ESP_017413_2300   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.67

230.

-12.

9.171

44.2

42.2

Polar Crater with Summer Ice:   ESP_017510_2465   ESP_017945_2465   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
66.39

99.7

-0.4

14.50

49.4

48.4

Impact Crater Exposing Stratigraphy in Eos Chasma:   ESP_017463_1630   ESP_018241_1630   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

315.

4.08

-7.28

63.1

65.0


  


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