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.

Unnamed Fresh Crater Northeast of Ascraeus Mons:   PSP_003844_1995   PSP_004134_1995   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.23

260.

-0.4

26.39

63.0

60.2

Cover a Subset of Gullies Previously Identified in MOC Image M10-03905:   PSP_004196_1325   PSP_005251_1325   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.2

19.4

-5.9

-28.1

44.3

43.4

Western Region of Zunil Crater:   PSP_004309_1880   ESP_020211_1880   (Interval in Earth days: 1239)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.728

166.

4.71

29.29

53.0

52.5

Interesting Gullies:   PSP_004176_1405   PSP_005587_1405   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.3

202.

8.88

-12.5

41.6

41.0

Layers and Fault in Crater in MOC Image R19-01820:   PSP_003168_1800   PSP_003880_1800   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.108

357.

-2.3

20.87

55.9

51.3

Relatively Large Primary Crater on Elysiu Planitia Young Lavas:   PSP_003267_1870   PSP_003412_1870   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.153

174.

-3.8

14.59

57.8

56.4

Gullies and Flow Features Along Crater Wall in Eastern Hellas Region:   PSP_003520_1405   PSP_005709_1405   (Interval in Earth days: 171)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.1

113.

0.37

-23.1

51.5

43.0

Ring and Cone Structures in Elysium Planitia North of Aeolis Planum:   PSP_003756_1825   PSP_004178_1825   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.521

144.

5.07

-8.42

54.3

52.1

Northwest Candor Mensa:   PSP_004186_1740   PSP_005597_1740   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.11

286.

0.29

-24.8

47.3

35.8

Sample Gigas Fossae:   PSP_003410_1840   PSP_003832_1840   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.778

230.

7.27

-6.05

55.8

55.2


  


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