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.

Terrain Southwest of Jovis Tholus:   ESP_088411_1960   ESP_088978_1960   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.96

239.

5.80

-9.01

47.5

49.9

Structure of Viscous Flow Feature Exposed by Ice Degradation:   ESP_088510_2220   ESP_088431_2220   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.58

51.9

11.0

-13.2

42.7

44.7

Dunes in Northern Mid-Latitude Crater:   ESP_088469_2410   ESP_088548_2410   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
60.69

87.7

5.29

19.86

47.3

46.3

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

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

Pitted Cones in Aurorae Chaos:   ESP_088540_1720   ESP_089107_1720   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.77

320.

3.86

-8.75

60.1

60.9

Jezero Crater:   ESP_088707_1985   ESP_088773_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.47

77.5

0.57

-21.6

47.7

49.7

Stunning Outcrop in Nilosyrtis Mensae:   ESP_088681_2160   ESP_088892_2160   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.47

65.6

-5.2

-14.7

44.7

46.4

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

Layering in Lucus Planum:   ESP_088769_1730   ESP_088980_1730   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.74

187.

5.48

-6.90

59.5

60.3


  


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