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.

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_088186_2175   ESP_088753_2175   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.39

260.

0.31

-14.6

42.8

45.7

Dune Monitoring in North Mid-Latitude Crater:   ESP_088311_2350   ESP_088377_2350   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.61

83.4

5.81

-7.40

45.0

46.2

Dune Monitoring in North Mid-Latitude Crater:   ESP_088261_2420   ESP_088182_2420   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.94

6.66

6.67

-7.68

47.4

48.6

Sinuous Channel near Pavonis Mons:   ESP_088358_1775   ESP_088569_1775   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.36

248.

13.3

-2.87

56.0

57.4

Channel South of Janssen Crater:   ESP_088168_1800   ESP_088458_1800   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.118

37.6

-7.2

12.15

55.4

54.8

Dune Field:   ESP_088035_2385   ESP_088378_2385   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
57.96

58.8

6.11

-24.3

45.9

48.8

Small Fresh Impact Crater:   ESP_088159_1670   ESP_088726_1670   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.0

283.

6.05

-15.1

62.5

64.7

Grooves and Undercutting in Columbia Valles:   ESP_088171_1705   ESP_088316_1705   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.60

316.

-5.9

3.691

61.1

60.9

Obstacle within Lobate Debris Apron:   ESP_088359_1435   ESP_088570_1435   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

225.

7.68

-5.73

78.9

79.8

Pits in North Polar Layered Deposits:   ESP_088394_2650   ESP_088367_2650   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.81

318.

-7.7

6.46

60.4

59.8


  


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