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.

Flow Draped over Crater Rim Visible in CTX Image :   ESP_025563_1975   ESP_025207_1975   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.48

209.

15.2

2.131

39.4

38.8

Fresh Crater on Northern Plains:   ESP_025775_2290   ESP_026065_2290   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.83

177.

8.09

25.59

41.9

39.7

Channel in Tharsis Region:   ESP_025417_1965   ESP_024916_1965   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.19

235.

17.6

-8.13

38.8

38.5

Banded Features in Hellas Region Visible in CTX Image :   ESP_025555_1360   ESP_025621_1360   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.9

78.0

-7.5

-22.6

77.3

78.9

Bedrock Exposed in the Central Uplift of a Unnamed Crater:   ESP_025766_2005   ESP_025700_2005   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.18

69.3

-7.5

11.70

41.5

39.7

Mesa-Forming Lobes Visible in CTX Image G07_020876_2133:   ESP_025623_2130   ESP_026335_2130   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.48

9.93

8.87

25.42

38.7

38.1

Hebrus Valles:   ESP_025777_1990   ESP_027254_1990   (Interval in Earth days: 115)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.14

127.

9.74

-19.1

40.7

47.4

Terrain with Parallel Lineations Visible in THEMIS Image V29600014:   ESP_025738_2195   ESP_026582_2195   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.24

110.

2.71

-14.2

40.0

42.0

Small Volcanoes Visible in THEMIS Image V27150023:   ESP_025773_2250   ESP_027039_2250   (Interval in Earth days: 99)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.61

233.

1.74

-18.1

41.1

44.3

Small Mounds in Chryse Planitia:   ESP_025427_1995   ESP_025282_1995   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.37

322.

6.11

-10.3

39.2

40.0


  


Page 579 of 873 (8,724 images)