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.

Alluvial Fans and Terraced Scarps in Kasei Valles:   ESP_088541_2025   ESP_088330_2025   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.38

291.

-19.

-6.13

47.7

46.0

Gullies on Western Wall of Nier Crater:   ESP_088574_2230   ESP_088640_2230   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.77

105.

-0.5

-17.0

44.0

45.8

Ridged Flow-Like Features in Deuteronilus Mensae:   ESP_088445_2225   ESP_088511_2225   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.33

26.8

8.67

-8.24

42.8

44.5

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088500_2435   ESP_088421_2435   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
62.98

320.

7.80

-6.45

48.1

49.1

Crater and Flow in Daedalia Planum:   ESP_088557_1685   ESP_089058_1685   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.5

217.

-8.9

3.217

63.3

62.3

Contact between Crater and Flood Lava:   ESP_088744_1845   ESP_089034_1845   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.224

148.

3.14

26.44

53.6

52.0

Layering and Contact in Lucus Planum:   ESP_088545_1725   ESP_088756_1725   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.43

184.

-3.0

-16.9

60.3

61.4

Stereo for Kunowsky Crater Dunefield:   ESP_088644_2370   ESP_088420_2370   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.72

350.

5.32

-16.7

46.6

47.9

Platy-Ridged Lava:   ESP_088635_2000   ESP_088780_2000   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.88

243.

-1.4

9.447

47.2

46.7

Escarpment Dune Field Topography:   ESP_088713_2640   ESP_088819_2640   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.92

233.

8.93

-5.01

59.8

60.9


  


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