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.

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

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

Thermally-Anomalous Crater on Hrad Vallis Flow:   ESP_017601_2145   ESP_018023_2145   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.20

141.

6.74

-6.84

40.9

43.0

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

Pits on Fan Surfaces in Mojave Crater:   ESP_017568_1870   ESP_018069_1870   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.120

326.

-6.1

13.95

49.9

49.5

Rim of 20-Kilometer Diameter Impact Crater in Eastern Isidis Planitia:   ESP_017629_1975   ESP_018051_1975   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.30

100.

-4.1

-19.7

45.5

47.7

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

Enigmatic Uplift on the Floor of Echus Chasma:   ESP_017306_1815   ESP_018084_1815   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.718

279.

5.93

-6.88

50.8

53.8

Multi-Pedestal Crater on Northern Plains:   ESP_017563_2375   ESP_018420_2375   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.98

95.7

-2.5

11.44

45.4

46.8


  


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