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.

Features in Echus Chasma:   ESP_068049_1805   ESP_072665_1805   (Interval in Earth days: 360)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.707

279.

4.52

27.80

41.1

54.4

Mesa with Bright Spot in Oxia Colles:   ESP_067849_2055   ESP_068245_2055   (Interval in Earth days: 31)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.41

333.

-12.

-24.5

49.3

48.5

Cross-Cutting Faults Southeast of Melas Chasma:   ESP_067732_1650   ESP_073746_1650   (Interval in Earth days: 468)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.9

290.

-14.

16.69

41.5

54.0

Troughs and Ridges in Chryse Planitia:   ESP_067823_2105   ESP_067480_2105   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.33

319.

13.9

-5.70

50.2

54.9

Collapse Terrain near Orson Welles Crater:   ESP_068061_1785   ESP_072677_1785   (Interval in Earth days: 360)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.50

313.

1.23

21.77

41.5

55.4

Crater Floor Outcrop:   ESP_067980_2160   ESP_063970_2160   (Interval in Earth days: 312)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.60

0.43

-22.

-12.2

54.5

59.7

Very Fresh Small Impact Crater:   ESP_067714_1815   ESP_076827_1815   (Interval in Earth days: 710)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.484

59.1

-5.1

8.893

40.7

36.3

Inverted Channel in Cusus Valles:   ESP_067833_1960   ESP_067965_1960   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.05

49.8

5.88

-3.77

43.8

44.2

Two Notches near Lowest Elevation Point of Crater Rim:   ESP_067821_1465   ESP_067689_1465   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

24.7

-7.3

6.887

48.4

45.5

Valleys in Crater Northeast of Argyre Region:   ESP_067704_1500   ESP_073784_1500   (Interval in Earth days: 474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

334.

7.13

20.86

44.0

53.7


  


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