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.

Channels with Tributaries on Rocky Plains Northwest of Argyre Region:   ESP_064645_1320   ESP_082568_1320   (Interval in Earth days: 1397)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.5

301.

5.97

-6.62

63.9

60.6

Blocky Terrain in Elysium Planitia:   ESP_064835_1830   ESP_090432_1830   (Interval in Earth days: 1994)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.193

147.

5.27

-16.6

58.1

57.9

Flow-Like Feature within Chryse Planitia:   ESP_064723_2000   ESP_072993_2000   (Interval in Earth days: 644)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.95

324.

-6.0

5.877

63.2

57.9

Flow-Like Feature within Chryse Planitia:   ESP_064868_2005   ESP_064156_2005   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.24

324.

13.0

-11.5

62.9

58.6

Eroded Crater near Lowell Crater:   ESP_064711_1325   ESP_065265_1325   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.1

300.

-0.9

-26.2

63.2

56.9

Landform in CTX Image G03_019466_2032_XN_23N014W:   ESP_064709_2035   ESP_072979_2035   (Interval in Earth days: 644)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.38

345.

-4.9

6.945

64.2

58.2

Inverted Channels:   ESP_064527_1440   ESP_055573_1440   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.6

280.

9.24

-8.74

61.2

60.4

Circular Landform North of Kasei Valles:   ESP_064869_2085   ESP_074972_2085   (Interval in Earth days: 787)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.06

296.

2.44

-23.2

66.9

68.6

Fractures in Chryse Planitia:   ESP_064855_2000   ESP_065765_2000   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.68

320.

-3.6

8.387

63.9

64.4

Layers along Hegemone Dorsum:   ESP_064605_1250   ESP_073587_1250   (Interval in Earth days: 700)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.8

314.

4.53

26.09

67.5

63.1


  


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