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.

Impressive Central Peak:   PSP_007555_1965   ESP_024354_1965   (Interval in Earth days: 1309)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.11

100.

-5.7

-26.8

41.4

38.6

Small Fresh Primary or Large Secondary Crater From Gratteri Crater:   PSP_007209_1565   PSP_008290_1565   (Interval in Earth days: 84)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.3

194.

-6.7

16.15

54.8

65.4

Preserved Fans in Unnamed Crater in Tartarus Region:   PSP_008093_1995   PSP_008383_1995   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.47

169.

-4.6

6.092

43.2

43.4

Faulted Layers in Impact Crater:   PSP_008023_1745   PSP_010238_1745   (Interval in Earth days: 173)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.29

284.

-3.7

13.99

53.0

57.2

Mawrth Vallis Phyllosilicates:   PSP_007019_1980   ESP_077041_1980   (Interval in Earth days: 5456)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.68

336.

0.65

16.95

38.6

38.7

Ring and Cone Structures in Grjota Valles:   PSP_007869_1960   PSP_007579_1960   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.90

164.

18.0

4.908

41.1

40.7

Olympus Mons North Scarp Detail:   PSP_007735_2030   PSP_008091_2030   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.92

224.

4.41

-5.92

40.5

42.5

Well-Preserved 15-Kilometer Diameter Crater Near Nili Fossae:   PSP_007912_2030   ESP_018342_2030   (Interval in Earth days: 813)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.63

71.3

0.11

15.86

41.5

43.9

Polar Crater with Summer Ice:   PSP_008081_2405   PSP_008793_2405   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
60.34

129.

4.55

-12.0

48.2

47.8

Small Craters in Amazonis Planitia:   PSP_008092_1980   PSP_008527_1980   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.87

197.

-5.7

8.084

43.7

44.3


  


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