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.

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

Kasei Valles Alluvial Fans:   ESP_088633_2040   ESP_088778_2040   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.55

298

-6.4

3.817

46.5

46.1

North Polar Layered Deposits Structural Geology in Icy Layers:   ESP_088733_2630   ESP_088562_2630   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.71

56.5

6.65

-7.41

59.1

59.3

Aeolis Dorsa Inverted Deposits:   ESP_088612_1735   ESP_088823_1735   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.35

154.

-1.4

-14.9

59.6

60.6

Channels along Hydraotes Chaos Channel:   ESP_088566_1835   ESP_088711_1835   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.377

329.

3.41

14.35

53.8

53.2

Fan-Shaped Feature in Ismenius Lacus:   ESP_088485_2145   ESP_088696_2145   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.95

17.5

-4.9

-15.7

44.2

45.9

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

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

Jezero Crater:   ESP_088562_1985   ESP_089208_1985   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.47

77.4

-8.9

15.11

48.1

47.9

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


  


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