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.

Possible Phyllosilicates Associated with Small Crater in Tyrrhena Terra:   ESP_077657_1665   ESP_076760_1665   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

89.1

0.02

14.13

49.1

37.1

Traverse Ramp in East Coprates Chasma:   ESP_077504_1640   ESP_076396_1640   (Interval in Earth days: 86)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

306.

1.04

-18.0

48.3

37.1

Crater in Arabia Terra:   ESP_077673_2240   ESP_077963_2240   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.77

4.07

5.25

16.62

47.2

44.6

Troughs and Ridges in Chryse Planitia:   ESP_077556_2155   ESP_077490_2155   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.40

321.

-8.2

7.351

45.3

44.4

Channels Intersecting Crater in Xanthe Terra:   ESP_077702_1755   ESP_076805_1755   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.60

301.

-27.

-7.96

47.8

37.6

Looking at the Crater Half Full:   ESP_076968_1475   ESP_076823_1475   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.4

173.

23.4

-6.17

48.0

47.6

Recent Crater:   ESP_077370_2130   ESP_077858_2130   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.80

357.

-2.7

-25.4

44.7

45.2

Alluvial Fan in Kasei Valles:   ESP_077148_2035   ESP_084809_2035   (Interval in Earth days: 597)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.42

296.

0.66

22.69

41.6

50.3

Ares Vallis:   ESP_077371_1930   ESP_077437_1930   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.93

331.

12.7

1.101

38.5

39.8

Pasted-on Material on Crater Ejecta:   ESP_077346_1845   ESP_077135_1845   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.419

294.

18.5

-6.08

38.2

38.9


  


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